第 213 期·中文精讀

巴里·巴里什:引力波與史上最精密的儀器

Barry Barish: Gravitational Waves and the Most Precise Device Ever Built

諾貝爾物理學獎得主講述 LIGO 如何捕捉時空漣漪,以及建造人類最精密儀器背後的工程難題與人生經歷。

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中文精讀由 AI 基於原始訪談改寫,非官方翻譯,可能存在偏差或錯誤;表述以原音訊與官方文稿為準。說明

LIGO 要測量的位移是 10 的負 18 次方米。一個質子的直徑大約 10 的負 15 次方米。這套儀器要感知的形變,比質子本身還小一千倍。

它由兩臺探測器組成,各自有兩條四公里長的真空管道,相距三千公里,同步執行。它們要捕捉的,是宇宙中最暴烈的災難在兩個黑洞合併時盪出的引力波。這個波從十三億光年外出發,到達地球時,已經把空間拉伸和擠壓到了極其微弱的程度。

巴里·巴里什(Barry Barish)因為這個裝置拿了 2017 年的諾貝爾物理學獎。他在 Lex Fridman 的播客裡聊了兩個多小時,談的東西從粒子物理一路走到俄羅斯文學,中間幾乎每一段都值得停下來想一想。

一個八歲小孩的問題

巴里什小時候是個“煩人精”,逮著父親問個不停。八歲那年他問了一個讓父親卡住的問題:冰是水做的,那它為什麼能浮在水上?

這個問題不新鮮,但它是他記憶裡父親第一次答不上來。從那一刻起,他明白了一件事:想回答自己的疑問,有別的辦法。去圖書館,去問懂更多的人,最後走到大家叫做研究的那條路上。

如果一個人會問好問題,又有解決問題的機制,那他做的就是我這一輩子在做的事。這未必是物理。這是人類身上極好的一種品質,我們該養著它。(巴里·巴里什)

他覺得教育系統恰恰在幹相反的事。小孩本來問個不停,大人嫌煩,叫他閉嘴。上學以後,學生被安排著唸書、做題,沒人鼓勵他們去煩別人。好奇心就這麼被磨掉了。

他自己是倖存者。他有點自嘲地說,可能是因為自己沒被修理乾淨,或者乾脆還沒長大。他後來在加州理工教本科,認為學生身上最大的短板就是好奇心不足,而好奇心本來是人天生就有的東西。

那段關於冰的記憶後面還有續集。他後來又好奇:下雨後地是溼的,過一會兒就幹了,水去哪了?再後來他學到,水由氫和氧組成,這倆都是氣體,那怎麼就變成了一種液體?這兩個問題他當時都答不出來,但答案後來一路把他領進了物理。

費米:最後一位雙棲的物理學家

巴里什高中在芝加哥讀,常去費米實驗室(Fermilab)上課,順便看野牛。他說恩里科·費米(Enrico Fermi)對他影響很大,理由很具體:費米是最後一位同時做實驗和做理論的重量級物理學家。

1933 年底,費米在幾個月內幹成了兩件大事。

第一件是寫下了貝塔衰變的理論。當時中子剛剛在 1932 年被發現,人們才知道原子核由中子和質子構成,外面繞著電子。費米憑空拿出一套理論,管用了幾十年,後人只是往上添補。他把論文投給《自然》(Nature),被拒了,理由是“太推測性”。他回到羅馬的辦公桌前把論文加長,改得更完整,然後投給了義大利和德國的本地物理期刊。這篇文章後來成了經典。

第二件是實驗。1934 年初,約里奧-居里夫婦(Frédéric Joliot 和 Irène Curie)第一次看到了人工放射性:用阿爾法粒子轟擊鋁,激發出某種會衰變、有半衰期的物質。這在當時意義極大。天然放射性材料稀少,但人工造出的放射性材料可以大量製造,醫學和工業都能用上。

費米的洞察在於:跟上這個實驗的正確方式,是用剛發現的中子當炮彈。帶正電的阿爾法粒子做不到這一點,中子不帶電,能直接鑽進核裡。這個想法在當時近乎異想天開,中子剛被發現,數量少得可憐。但他還是做成了,這項實驗工作為他拿下了諾貝爾獎,也邁出了通往核裂變的第一步。

他甚至很快發現,慢中子比快中子更好用。這是在實驗裡摸出來的經驗。

巴里什說這件事被記住了很多年,因為它幾乎無法複製。從那以後,再沒有人能同時在理論和實驗兩端都做到這種高度。他自己年輕時也想成為費米那樣的人,結果只做到了一半的一半:他做的實驗,始終跟理論貼得很近。

好奇心是一把帶棘輪的刀

費米的政治立場相當淡漠。從他自己留下的文字、他太太的回憶、旁人的記述看,他基本只用科學家的眼光看世界。但他參與了曼哈頓計劃,原子彈落在了日本。巴里什說他不想把這件事當成自己的遺產。

巴里什提到一本叫《好奇心的棘輪》(The Ratchet of Curiosity)的書。棘輪只朝一個方向轉。知識也一樣,你知道了,就回不去。你想看看會發生什麼,然後真的發生了什麼,有時候你控制不住。

Lex 把話題接了過去。他說人工智慧眼下就處在同一道口子上:你把系統放出去,抱著希望看它怎麼運轉,大多數情況下因為系統還不夠強,壞事沒發生。但同樣這股好奇心往前推,可能推到某個毀滅性的結果。生物工程也一樣。巴里什認同,他說這是同一個邏輯在不同領域重複。

他沒給答案。他只是承認,這門功課人類一直沒有學好:怎樣在求知的同時守住底線。

愛因斯坦寫錯過兩次

談引力波之前,巴里什把物理史捋了一遍。

牛頓給了萬有引力的公式,力正比於兩個質量的乘積,反比於距離的平方,前面掛一個常數 G。這套理論管用了兩百多年,沒人找到違反它的例子。但牛頓沒解釋為什麼蘋果會被地球吸引。他只描述了現象,沒講機制。

水星軌道有個小小的偏差,用牛頓理論算不對。這個偏差最後由愛因斯坦(Albert Einstein)修掉了。1915 年,愛因斯坦拿出廣義相對論,這是一套全新的引力理論。他為了這個理論整整磨了十年,儘管 1905 年那一年他幾個月之內解決了物理學的三四個大問題。

1916 年,愛因斯坦又寫了一篇小論文。他沒做複雜推導,用的是直覺。他發現,如果把廣義相對論的公式用一種特定的方式寫下來,它跟電磁學的公式長得很像。電磁學裡,二十多年前剛發現它有波,也就是光、無線電、各種輻射。於是他跳了一步:既然公式像,引力大概也有波。

巴里什說,這一步跳得非常大。

那篇論文寫得並不好,還帶著一個嚴重錯誤:引力強度算錯了一個因子 2。愛因斯坦沒承認,兩年後直接重寫一篇把錯誤改掉。第二篇論文裡,他還說清了引力波怎麼產生:電磁波用一個正電荷和一個負電荷來回振盪就能造出來,這是偶極矩;引力波不行,它需要四極矩,得是三維空間裡的振盪才成。依然是靠直覺,沒有推導。

同一個年份,施瓦西(Karl Schwarzschild)提出了黑洞。巴里什說這一點挺有意思:黑洞這個念頭來自施瓦西,愛因斯坦本人沒有提出來。施瓦西是德國理論物理學家,兩年後死在一戰裡。

一場三十年的爭論

廣義相對論太難了。四維,不像三維那麼直觀,座標選不好就會冒出無窮大,大家叫它座標奇點。愛因斯坦自己被這個坑絆住過。

1932 年他到美國,1935 年前後跟羅森(Nathan Rosen)一起回頭看這個問題。他試著從廣義相對論裡重新推出引力波,一路推,一路撞上無窮大。1936 年,兩人寫了一篇論文投給《物理評論》(Physical Review),標題相當擰巴:《引力波存在嗎?》。他二十年前就提出這東西存在,現在又反過來質疑。

當時的編輯叫泰特(John Tate),很年輕,後來做了很多年編輯。他把稿子送去了外審,審稿人是羅伯遜(Howard P. Robertson),正好在加州理工休假,平時在普林斯頓,跟愛因斯坦是同事。羅伯遜看出了問題:座標選得不對,才會冒出這些無窮大。他順手給了一個示範,換成柱座標,無窮大就沒了。

泰特給愛因斯坦回了封信,措辭委婉,大意是“您怎麼看我們審稿人的意見”。愛因斯坦的回信被完整記錄下來:我把論文寄給你是為了發表,不是讓你送給什麼所謂的專家看。我撤回。此後他再也沒在《物理評論》上發過文章。

他把論文改寫,換了標題,發在費城富蘭克林研究所的刊物上。這是愛因斯坦最後一次公開寫引力波。

爭論一直到 1958 年才收口。那年開了一場會,把廣義相對論的行家都叫來,英國一位理論學家從理論核心出發給出了完整推導,引力波確實存在。會上還有理查德·費曼(Richard Feynman)。費曼說了句很費曼的話:如果引力波真的存在,它得能幹點什麼事,否則就不算存在,它得能傳遞能量。他順手想了一個思想實驗:一根棒子,上面套幾個環,引力波過去,棒子發生畸變,帶動環摩擦生熱,能量就這麼傳過去了。

這條思路上到這一步,理論界基本接受了。剩下的問題只剩一個:訊號太弱,弱到幾乎不可能測。

比質子小一千倍的形變

引力波經過時,空間會一個方向被拉長,另一個方向被壓短,來回交替。巴里什打了個比方:你去遊樂園照哈哈鏡,一面鏡子把你照得又矮又胖,旁邊那面把你照得又高又瘦。你在一秒鐘之內來回走一趟,就是一個週期一秒的引力波。走六十趟,頻率就是六十赫茲。

差別只在幅度。而幅度小到荒謬。

LIGO 要測的拉伸量是 十的負二十一次方。臂長四公里,乘上去,需要測到的位移是十的負十八次方米。這就是那個比質子小一千倍的數。

用什麼測?干涉儀。一束鐳射一分為二,各走一條垂直的臂,盡頭是鏡子,反射回來。如果兩條臂一樣長,回來的光反相一疊加就互相抵消,什麼都看不到。如果其中一條被引力波拉長了一點點,回來的時間就對不齊,抵消不完全,訊號出現了。

原理聽著簡單,做起來是另一回事。真正的難點全都是工程。

世界上最貴的減震器和降噪耳機

第一個問題:地震。地球每時每刻都在動。你把一個測到十的負十八次方米的儀器直接放在地上,它什麼也測不出來。

解決辦法是巴里什口中“世界上最花哨的減震器”。汽車裡只有一層,這裡有四層疊起來。每層裡填的是恰當“軟硬度”的材料,形狀像小彈簧。頭一層擋住一部分振動,剩下的交給第二、第三、第四層。

四層不夠。他們又加了一樣東西,你還是熟悉的:主動降噪。原理跟飛機上戴的 Bose 耳機一樣。耳機感受發動機的持續噪聲,反向抵消掉,乘務員來問你要咖啡還是茶的時候,你聽得很清楚,因為那是訊號,不是環境。

LIGO 裡做的比這難。它不光要知道有噪聲,還得知道噪聲從哪個方向來。他們在減震器陣列裡再放一圈地震儀,測殘餘的運動和方向,然後佈置小的執行器反向推回去。最後:地面上傳進來的震動被壓到了原本的十的負十二次方。

Lex 當時說了一句:這是有史以來最精密的機器人。巴里什沒否認。

第二個問題:真空。整套裝置必須在真空裡跑,兩條四公里長的管道,是全世界最大的高真空系統。做管子的辦法是從一卷不鏽鋼開始,像捲紙一樣螺旋卷出來再焊上,焊縫也是螺旋的。

讓他們這些年一直擔心的是漏氣。普通實驗室裡,檢測漏氣的方式是拿氦氣包圍被測物,看氦從哪兒鑽進來。四公里的管子沒法用氦包圍。真空度本身可以測,但一旦哪裡裂了,怎麼找、怎麼修,一直是懸在頭上的問題。

十年,什麼也沒看到

1994 年,美國國家科學基金會(NSF)批了錢。造了五年,1999 年基本單元搭起來。那時的版本還沒有主動隔震,也沒有後來的一些關鍵能力。

他們做的第一件事是隻用有把握的技術,先在實驗室裡跑通。儀器搭好、能動,但動得不好。看不到引力波。

接下來是接近十年的迴圈:開機跑上幾個月找訊號,什麼都沒看到,回頭搞清楚瓶頸在哪,修上幾個月,再開機。年年如此。

直到他們確認必須做一次大改。加進主動隔震,改掉一批別的設計缺陷。NSF 又給了大約一億美元。改完,2015 年重啟,幾乎立刻看到了兩個黑洞的第一次碰撞。

剩下的事情反而是最謹慎的部分。訊號太像理論預測了,反而要防著點。

巴里什說,團隊裡不少人當場就信了。圖上一半是原始資料,另一半是愛因斯坦方程的數值解,幾乎重合,還是兩臺相隔三千公里的探測器同時看到的。這已經相當有說服力,但科學家不能騙自己。他們得先確認新改過的儀器本身不會造出這種形狀的訊號,這需要測試。第二件更要緊的事:得確認自己沒被黑進來。哪怕儀器不接網際網路,物理接觸也是可能的。Lex 說這是網路安全問題,巴里什說對。

一個月之內,內部說服了自己。一千多名合作者一聲沒吭。

Lex 說這件事最能說明團隊的凝聚力。要麼是鐵板一塊,要麼是很強的紀律。巴里什笑,說統治可以靠怕,也可以靠愛,這個道理馬基雅維利早就寫過了。

又過了一個月,他們才把看到的東西徹底弄明白,做到能真正用它做科學,把解讀留在自己手裡。

一千人的團隊怎麼運轉

一百多人的起點,最後變成一千多人。怎麼帶?

巴里什的說法很樸素:目標是讓整體的結果大於各部分之和。這話誰都會說,但他說出了裡面的門道:把一堆人和想法直接摞在一起,結果通常小於總和,因為大家重疊了。想讓結果超過總和,就得設計出一種結構,讓某些事單靠一個人根本做不成,必須幾種能力湊在一起才成。

然後關鍵在哪?

最難的一步,是把世界上最好的人吸引過來,讓他們願意為此花上好幾年。唯一的辦法,是讓他們相信,在這裡做的事比他們自己能單獨做的更有意思。(巴里·巴里什)

最難管的是什麼?自我。他說這靠手藝,科學的方法在這裡不太管用。

他舉了一個例子。LIGO 需要的鐳射器是一種很特殊的型號,全世界只有三家機構有這方面專家,彼此還在賽跑。巴里什的辦法是把三家都請進來一起做。對他們來說,這是第一次在同一個裝置上跟對手合作,而且自己成了這支更大隊伍的一部分,能碰到單幹碰不到的東西。

另一件小事更見功夫:發論文的時候,一千多號人得對某一個句子的措辭、對標題的寫法達成一致。這件事的意義在於,讓每個人真心覺得自己是貢獻者的一部分。

愛因斯坦和希格斯的不同命運

引力波探測器把一個新領域開啟了。用巴里什的話說,關機之前,幾乎每週都能看到一個引力波事件。等明年重啟,預計會變成每兩天一次。而且事件型別各不相同。

他拿這跟希格斯玻色子做對比。歐洲核子研究中心(CERN)那臺巨大的加速器發現了希格斯,那是一次偉大的發現。但發現之後,想再往前推就很吃力。原因在於,加速器裡的物理背景太厚了,你想看出一個新東西,得從一大堆別的物理現象裡把它扒出來。這些背景本身就是物理,甩不掉。

LIGO 的處境不一樣。它面對的背景來自技術,跟物理無關。

訊號微弱,這是真的。但只要把地球的震動隔得更乾淨,把鐳射做得更強,訊號就會從背景裡露出來。背景是會變的,會隨著你的手藝變好而退下去。這就是為什麼巴里什說,LIGO 的極限不在物理,在工程。只要物理沒給你劃線,工程師早晚能把它造出來。

他提到伽利略。伽利略之前就有人造出望遠鏡,但他把望遠鏡做成了一種研究工具,看向天空,看到了木星的衛星。那是用眼睛之外的東西看宇宙的開始。此後幾百年,望遠鏡越做越好,天文學一路走下去。引力波天文學現在也是剛學會爬。

再往後一步,是把靈敏度再提升十倍。十倍靈敏度意味著能看遠十倍,看遠十倍就是可觀測體積擴大一千倍。再往後,就是宇宙學了。

光學望遠鏡只能看到宇宙三十八萬年之後的東西,因為在那之前,宇宙太密,光子出不來。引力波不受這個限制,它從更早就能穿出來。原則上,我們能用引力波去看宇宙最初的樣子,去看大爆炸本身是什麼。

為什麼宇宙裡沒有反物質

物理學上有個尷尬的問題,巴里什把它拎出來專門講了一遍。在實驗室裡把能量撞成物質,你得到多少物質,就得到多少反物質。物質和反物質相遇會湮滅,重新變回能量。

那麼早期的宇宙裡,物質和反物質應該一樣多,然後互相消滅掉。結果應該什麼都不剩。但我們看到的是滿宇宙都是物質,反物質幾乎找不到,除非去實驗室裡造。

這說明早期的宇宙裡本來存在某種不對稱,物質比反物質多了一點點。我們不知道那是什麼。現有的物理沒有能力解釋為什麼我們在這裡。(巴里·巴里什)

這裡問的是物理問題,跟哲學意義上的“為什麼活著”無關:等式兩邊對不上,少了一項。

Lex 問了個外行問題:反物質有引力場嗎?能不能透過引力訊號去研究這種不對稱?巴里什說原則上,如果存在反中子星,我們應該能看到不同形式的訊號,但事情沒走到那一步。我們往哪兒看都是普通物質。宇宙裡做過的事,遠比我們在實驗室裡能做的多。

黑洞是什麼

黑洞是一個區域,時空彎曲到極強的地方,任何東西都逃不出去,包括光。光會被彎,彎到回不到外面。

它是怎麼來的?最容易想到的路徑是恆星死亡。恆星靠核聚變燃燒,把氫燒成氦,再一路往上燒更重的元素,燒到鐵就燒不動了。恆星一直處在兩種力的拉鋸裡:往外是核聚變的壓力,往裡是引力。燒完,往外的那股力沒了,整顆星向裡塌,這就是超新星。

塌下來之後,如果原來是顆足夠大的星,引力場能強到形成黑洞。我們的太陽不行,太小。通常的說法是需要至少三倍太陽質量。這只是最主流的一種解釋,未必對。

LIGO 看到過一些不太符合這套解釋的東西。最重的一個系統,合起來是一百四十倍太陽質量。這麼大的恆星被認為不穩定,不應該存在。它們可能由小黑洞互相吞併慢慢長大,也可能來自更早,是大爆炸時直接造出來的原初黑洞。如果真的有一大批原初黑洞,那它們可能就構成了暗物質的一部分。

哪一種是真相,現在還分不出來。但引力波給了一條線索:測量它們的質量分佈、自旋方式、系統有沒有搖晃,看數量隨時間怎麼變。這些資料會慢慢指路。

巴里什說黑洞最迷人的地方不只是天體。它是唯一一個量子場論和廣義相對論必須同時出場的地方。到今天為止,這是物理學最大的尷尬之一:我們手上有兩套極好的理論,一套描述微觀世界,一套描述高速和大尺度,但兩套拼不起來。人們尋找統一理論找了幾十年,主要是從數學入手,進展不大。巴里什說他相信得先有實驗線索。而黑洞內部,可能就是那個線索出現的地方。

他提到弦理論。弦理論在數學上很漂亮,但它要求十一維。要得到我們這個世界裡的預測,就得把多出來的七維處理掉,辦法是假設它們捲曲在極小尺度上。這個做法在數學上說得通,但做法不唯一。不唯一的代價就是沒有預測能力,對物理來說這是致命的。

費米悖論與光速的牢籠

費米留下來一句著名的話。他和泰勒(Edward Teller)、約克(Herb York)一起吃午飯,坐下來問了一句:他們在哪兒?

意思很明白:按機率算,宇宙裡有那麼多星系、恆星、行星,智慧生命不應該只有我們一家。那為什麼一點動靜都沒有?後來德雷克(Frank Drake)把這套推算整理得更細,結論還是那個方向:如果只有我們,那才叫奇蹟。

巴里什的看法平實:生命很可能存在,智慧生命大機率也有。但溝通這件事,比大家想象的難。所有我們知道的通訊方式都跑在光速上,光速還限制不了往返對話。訊號發出去沒問題,但要形成交流,得兩邊離得足夠近,近到光速還來得及週轉。

Lex 追問:那有沒有可能用引力來通訊?巴里什說,為什麼不能。只是對我們來說,探測引力效應極難,得是黑洞那個量級的東西才行。人類目前還很原始。他提到自己一些很受尊敬的同行,一輩子都在找一種“第五種力”,也許那才是關鍵。這第五種力可能作用距離更長,不像引力那樣按平方反比衰減。

南極站是火星的預演

他們聊到星際擴張。巴里什覺得這還很未來。但一次去火星的單程旅行,他說並不遙不可及,問題只在於有沒有人願意去。而願意去的人從來不缺。

他自己去過南極。當年作為國家科學委員會成員去的,沿路是:美國飛澳大利亞,再到基督城,然後坐軍用飛機飛七八個小時到麥克默多站(McMurdo Station),那是個沿海站,有一千多人。飛行員飛到一半在廣播裡說,抱歉,這趟叫回旋鏢飛行,天氣不允許降落就得原路返回。他們還真返回了一次。之後再飛,再從麥克默多飛到南極點。

南極點當時是零下五十一度,那是夏天。海拔約一萬一千英尺,因為溫度永遠低到雪融不了,雪一層層堆上去。極度乾燥,幾乎零溼度,身體得慢慢調適。那站上不到一百人,他去的時候五六十人,冬天只剩一半。

Lex 把話題引到火星備份上。他說南極站可以類比:我們沒有殖民南極,因為全是冰和寒,但我們建了站。區別在於,火星是一個異地備份。如果地球出了事,別處還留有人類。

巴里什沒反駁。他說我們目前在南極也就做到這一步,沿海的麥克默多站有溫室,能自給,再往裡就沒走遠。至於更遠的殖民,他只能說,那還很遠。

被《白鯨》勸退的作家夢

巴里什年輕時想當作家。家裡沒人上過大學,也沒人給他指路,他就是愛看書。母親讀的是推理小說,他很快讀膩了,十二三歲開始讀真正的文學。他說再沒有比俄羅斯文學更好的。

他讀了不少陀思妥耶夫斯基(Fyodor Dostoevsky)。在他眼裡,陀思妥耶夫斯基有兩點開創性:一是復調敘事,他是第一個嚴肅使用多重敘述者的作家;二是他是存在主義文學的開端。疫情期間他重讀了加繆(Albert Camus)的《瘟疫》(The Plague),他說那是一本講愛的書,愛的是人類,在這個時間讀非常合適。

他最喜歡的一本是《白痴》(The Idiot)。書裡的梅什金公爵(Prince Myshkin)像個不屬於這個世界的人。巴里什說自己常自稱白痴,因為對這個世界的理解總是幼稚,這也許有遺傳成分。他和這個角色有點精神上的連線。

索爾仁尼琴(Aleksandr Solzhenitsyn)給他的東西不一樣。他從書裡讀到的是人性的殘忍和冷漠,也讀到人能在最微小的樂趣裡找到活下去的理由。在勞改營裡能把一天過完還覺得過得去,這件事本身就很驚人。他加了一句自己的觀察:作惡最有效的方式,是讓人相信自己在做好事。斯大林很可能真心認為自己是在為世界謀福。古拉格就是這句話最清晰的註腳。

他提到一位近五年拿諾貝爾文學獎的作家(指阿列克謝耶維奇 Svetlana Alexievich),採訪物件是各種年齡、各種職業的人,回憶蘇聯時期的經歷。有意思的是,很多人回頭看,覺得過去更好。

然後就是那個笑話。他高中讀了一門最嚴肅的文學課,讀了《白鯨》(Moby Dick),結果把自己當小說家的念頭讀沒了。他當年讀到那關於鯨魚的長篇描寫,覺得太枯燥了,心想,如果這就是偉大的文學,那算了。三十多歲再讀,他明白了問題出在哪:《白鯨》是一整本書的隱喻,而十五歲的他連“隱喻”這個詞的含義都不清楚,一直在想“我為什麼要關心一條魚”。他說那本書本身是好的,問題在於他當時太小,讀不懂。

意義是給別人留下點什麼

Lex 問了個大問題:這一切到底有什麼意義?

巴里什說他大概不擅長回答哲學層面的問題。但他的個人版本是:你是不是對自己之外的東西造成了一點積極的改變。可能是對別人有用,可能是做出了引力波這樣的發現,落點在你自己生存範圍之外。你的生命因此有了意義。他說這話很樸素,但這差不多就是他能給出的最好回答。

被問到死亡,他說不怕,只是遺憾。他清楚自己已經過了大半輩子,仍然享受活著的狀態。他也能設想一種病到不想活的情況,但現在沒有。他說,這一趟走得不錯,不希望它結束,也談不上恐懼死本身。

Lex 說,正是有限性讓它特別,也正是它的不確定讓人不安。巴里什說他更在意的是生命的謎,尤其意識。我們能理解生命的大部分機制,但意識是另一回事,你能思考這件事本身,這件事他到現在都覺得難以對付。

被問到希望留下什麼,他說希望別人評價他的時候,覺得他推動了科學往前走,也算是一個像樣的樣板,教人該怎麼活。

至於那個裝置本身,用 Lex 的話說,它是人類集體最好的樣本:它出自一群人,憑一個人的力量做不出來。

海森堡(Werner Heisenberg)那句話可以借來收尾:宇宙不僅比我們想象的更奇怪,而且比我們能夠想象的更奇怪。

把這篇裡的東西用起來

  • 把自己那個“冰為什麼浮在水上”的問題記下來。巴里什的科研起點是父親答不上來的一個問題。你現在答不出來的問題裡,可能有一個就是你未來十年最值得追的東西。
  • 刻意找一件不重疊的合作。巴里什管理一千多人的辦法是讓“整體大於部分之和”。如果你正在帶團隊,檢查一下:你安排的任務裡,哪些是拼裝式的,哪些是必須靠兩類不同能力咬合才能做成的?後者才是團隊的槓桿。
  • 分清你的瓶頸是物理還是技術。LIGO 能一路往前走,是因為它的限制來自工程,不來自自然規律。做產品、做研究、找工作都是這樣。往前走一步撞到物理,掉頭;撞到技術,接著啃。
  • 把噪音和訊號分開看。主動降噪的邏輯是:先辨認出重複出現的背景,把它反向抵消。日常工作裡也一樣,先分清楚哪些是每週都重複的干擾,哪些是真正要處理的訊號,然後對第一類做減法。
  • 重讀一本你當年讀不下去的書。巴里什十五歲讀《白鯨》棄書,三十多歲再讀,發現當年缺的是“隱喻”這個概念。過幾年回頭看一些當時覺得枯燥的東西,你可能會發現變的是你自己。
  • 給衡量人生意義換一個指標。不用問“我得到了什麼”,問“我對自己之外的東西做了什麼”。巴里什的諾貝爾獎來自一個比質子小一千倍的測量,而這個測量最終屬於全人類。
文稿來自公開 Kaggle 資料集(rajneesh231/lex-fridman-podcast-transcript),為早期自動轉錄存檔,可能存在識別錯誤。
The following is a conversation with Barry Barish, a theoretical physicist at Caltech and the winner of the Nobel Prize in Physics for his contributions to the LIGO detector and the observation of gravitational waves. LIGO, or the Laser Interferometer Gravitational Wave Observatory, is probably the most precise measurement device ever built by humans. It consists of two detectors with four kilometer long vacuum chambers situated three thousand kilometers apart, operating in unison to measure a motion that is ten thousand times smaller than the width of a proton. It is the smallest measurement ever attempted by science, a measurement of gravitational waves caused by the most violent and cataclysmic events in the universe, occurring over tens of millions of light years away. To support this podcast, please check out our sponsors in the description. This is the Lex Friedman Podcast and here is my conversation with Barry Barish. Yeah, that memory is kind of something I use to illustrate something I think is common in science, that people that do science somehow have maintained something that kids always have. A small kid, eight years old or so, asks you so many questions usually, typically, that you consider them pests. You tell them to stop asking so many questions. And somehow our system manages to kill that in most people. So in school, we make people study and do their things, but not to pester them by asking too many questions. And I think, not just myself, but I think it's typical of scientists like myself that have somehow escaped that. Maybe we're still children or maybe we somehow didn't get it beaten out of us. But I teach it in college level and it's, to me, one of the biggest deficits is the lack of curiosity, if you want, that we've beaten out of them because I think it's an innate human quality. Is there some advice or insights you can give to how to keep that flame of curiosity going? I think it's a problem of both parents and that parents should realize that's a great quality we have. That you're curious and that's good. Instead, we have expressions like curiosity killed the cat and more. But basically, it's not thought to be a good thing. Curiosity killed the cat means if you're too curious, you get in trouble. I don't like cats anyway, so maybe it's a good thing. Yeah. That, to me, needs to be solved, really, in education and in homes. It's a realization that there's certain human qualities that we should try to build on and not destroy. One of them is curiosity. Anyway, back to me and curiosity. I was a pest and asked a lot of questions. My father generally could answer them at that age. And the first one I remember that he couldn't answer was not a very original question, but basically that ice is made out of water, and so why does it float on water? He couldn't answer it. It may not have been the first question. It's the first one that I remember. And that was the first time that I realized that to learn and answer your own curiosity or questions, there's various mechanisms. In this case, it was going to the library or asking people who know more and so forth. But eventually, you do it by what we call research. But it's driven by, hopefully, you ask good questions. If you ask good questions and you have the mechanism to solve them, then you do what I do in life, basically, not necessarily physics. And it's a great quality in humans, and we should nurture it. Do you remember any other kind of in high school, maybe early college, more basic physics ideas that sparked your curiosity or mathematics or science in general? I wasn't really into science until I got to college, to be honest with you. But just staying with water for a minute, I remember that I was curious what happens to water. It rains and there's water in a wet pavement, and then the pavement dries out. What happened to this water that came down? And I didn't know that much. And then eventually, I learned in chemistry or something, water is made out of hydrogen and oxygen. Those are both gases. So how the heck does it make this substance? It's liquid. Yeah, so that has to do with states of matter. I know perhaps LIGO and the thing for which you've gotten the Nobel Prize and the things much of your life work perhaps was a happy accident in some sense in the early days. But is there a moment where you looked up to the stars and also, the same way you wondered about water, wondered about some of the things that are out there in the universe? Oh, yeah, I think everybody looks and is in awe and is curious about what it is out there. And as I learned more, I learned, of course, that we don't know very much about what's there. And the more we learn, the more we know we don't know. I mean, we don't know what the majority of anything is out there. It's all what we call dark matter and dark energy. And that's one of the big questions. When I was a student, those weren't questions. So we even know less, in a sense, the more we look. So of course, I think that's one of the areas that almost it's universal. People see the sky, they see the stars and they're beautiful and see it looks different on different nights. And it's a curiosity that we all have. What are some questions about the universe that in the same way that you felt about the ice that today? You mentioned to me offline, you're teaching a course on the frontiers of science, frontiers of physics. What are some questions outside the ones we'll probably talk about that kind of, yeah, fill you with the, get your flame of curiosity up and firing up, you know, fill you with awe? Well, first, I'm a physicist, not an astronomer. So I'm interested in the physical phenomenon, really. So the question of dark matter and dark energy, which we probably won't talk about, our recent last 20, 30 years, certainly dark energy. Dark energy is a complete puzzle. It goes against what you will ask me about, which is general relativity and Einstein's general relativity. It basically takes something that he thought was what he called a constant, which isn't. And if that's even the right theory, and it represents most of the universe. And then we have something called dark matter, and there's good reason to believe it might be an exotic form of particles. And that is something I've always worked on, on particle accelerators and so forth. And it's a big puzzle, what it is. It's a bit of a cottage industry in that there's lots and lots of searches, but it may be a little bit like, you know, looking for a treasure under rocks or something. You don't, it's hard to, we don't have really good guidance, except that we have very, very good information that is pervasive and it's there. And that it's probably particles, small, that the evidence is all of those things. But then the most logical solution doesn't seem to work, something called supersymmetry. And do you think the answer could be something very complicated? You know, I like to hope that, think that most things that appear complicated are actually simple if you really understand them. I think we just don't know at the present time, and it isn't something that affects us. It does affect, it affects how the stars go around each other and so forth, because we detect that there's missing gravity, but it doesn't affect everyday life at all. I tend to think and expect maybe, and that the answers will be simple. We just haven't found it yet. Do you think those answers might change the way we see other sources of gravity, black holes, the way we see the parts of the universe that we do study? It's conceivable. The black holes that we've found in our experiment, we're trying now to understand the origin of those. It's conceivable, but doesn't seem the most likely that they were primordial, that is, they were made at the beginning. And in that sense, they could represent at least part of the dark matter. So there can be connections, dark black holes or how many there are, how much of the mass they encompass is still pretty primitive. We don't know. So before I talk to you more about black holes, let me take a step back to, I actually went to high school in Chicago and would go to take classes at Fermilab, watch the buffalo and so on. So let me ask about, you mentioned that Enrico for me was somebody who was inspiring to you in a certain kind of way. Why is that? Can you speak to that? Sure. He was amazing, actually. He's the last, I'll come to the reason in a minute, but he had a big influence on me at a young age. But he was the last physicist of note that was both an experimental physicist and a theorist at the same time. And he did two amazing things within months in 1933. We didn't really know what the nucleus was, what radioactive decay was, what beta decay was when electrons come out of a nucleus. And near the end of 1933, the neutron had just been discovered. And that meant that we knew a little bit more about what the nucleus is, that it's made out of neutrons and protons. The neutron wasn't discovered till 1932. And then once we discovered that there was a neutron and proton and they made the nucleus and then their electrons that go around, the basic ingredients were there. And he wrote down not only just the theory, a theory, but a theory that lasted decades and has only been improved on of beta decay, that is, the radiation. He did this, came out of nowhere, and it was a fantastic theory. He submitted it to Nature magazine, which was the primary best place to publish even then. And it got rejected as being too speculative. And so he went back to his drawing board in Rome where he was, added some to it, made it even longer, because it's really a classic article, and then published it in the local Italian journal for physics and the German one. At the same time, in January of 1932, Giulio and Curie, for the first time, saw artificial radioactivity. This was an important discovery because radioactivity had been discovered much earlier. They had x rays and you shouldn't be using them, but there was radioactivity. People knew it was useful for medicine. But radioactive materials are hard to find, and so it wasn't prevalent. But if you could make them, they had great use. And Giulio and Curie were able to bombard aluminum or something with alpha particles and find that they excited something that decayed and had some half life and so forth, meaning it was artificial version, or let's call it not a natural version, an induced version of radioactive materials. And Fermi somehow had the insight, and I still can't see where he got it, that the right way to follow that up was not using charged particles like alphas and so forth, but use these newly discovered neutrons as the bombarding particle. It seemed impossible they barely had been seen. It was hard to get very many of them. But it had the advantage that they're not charged, so they go right into the nucleus. And that turned out to be the experimental work that he did that won him the Nobel Prize. And it was the first step in fission, discovery of fission. And he did this two completely different things, an experiment that was a great idea and a tremendous implementation, because how do you get enough neutrons? And then he learned quickly that not only do you want neutrons, but you want really slow ones. He learned that experimentally, and he learned how to make slow ones, and then they were able to go through the go through the periodic table and make lots of particles. He missed on fission at the moment, but he had the basic information, and then fission follows soon after that. Forgive me for not knowing, but is the birth of the idea of bombarding with neutrons, is that an experimental idea? Was it born out of an experiment? Did he just observe something, or is this an Einstein style idea where you come up from basic intuition? I think it took a combination, because he realized that neutrons had a characteristic that would allow them to go all the way into the nucleus when we didn't really understand what the structure was of all this. So that took an understanding or recognition of the physics itself of how a neutron interacts compared to, say, an alpha particle that Julio and Curie had used. And then he had to invent a way to have enough neutrons, and he had a team of associates, and he pulled it off quite quickly. So it was pretty astounding. And probably, maybe you can speak to it, his ability to put together the engineering aspects of great experiments and doing the theory, they probably fed each other. I wonder, can you speak to why we don't see more of that? Is that just really difficult to do? It's difficult to do. Yeah, I think in both theory and experiment in physics anyway, it was conceivable if you had the right person to do it, and no one's been able to do it since. So I had the dream that that was what I was going to be like, Fermi. But you love both sides of it, the theory. Yeah, I never liked the idea that you did experiments without really understanding the theory, or the theory should be related very closely to experiments. And so I've always done experimental work that was closely related to the theoretical ideas. I think I told you I'm Russian, so I'm going to ask some romantic questions. But is it tragic to you that he's seen as the architect of the nuclear age, that some of his creations led to potentially, some of his work has led to potentially still the destruction of the human species, some of the most destructive weapons? Yeah, I think even more general than him, I gave you all the virtues of curiosity a few minutes ago. There's an interesting book called The Ratchet of Curiosity. A ratchet is something that goes in one direction. And that is written by a guy who's probably a sociologist or philosopher or something. And he picks on this particular problem, but other ones. And that is the danger of knowledge, basically. You're curious, you learn something. So it's a little bit like curiosity killed the cat. You have to be worried about whether you can handle new information that you get. So in this case, the new information had to do with really understanding nuclear physics. And that information, maybe we didn't have the sophistication to know how to keep it under control. And Fermi himself was a very apolitical person. So he wasn't very driven by, or at least he appears in all of his writing, the writing of his wife, the interactions that others had with him. Either he avoided it all or he was pretty apolitical. I mean, he just saw the world through kind of the lens of a scientist. But he asked if it's tragic. The bomb was tragic, certainly on Japan. And he had a role in that. So I wouldn't want it as my legacy, for example. But brought it to the human species that it's the ratchet of curiosity that we do stuff just to see what happens. That curiosity, that in sort of my area of artificial intelligence, that's been a concern. On a small scale, on a silly scale, perhaps currently, there's constantly unintended consequences. You create a system and you put it out there and you have intuitions about how it will work. You have hopes how it will work, but you put it out there just to see what happens. And in most cases, because artificial intelligence is currently not super powerful, it doesn't create a large scale negative effects, but that same curiosity as it progresses might lead to something that destroys the human species. And the same may be true for bioengineering. right. So we also work at this frequency. So we basically, why don't we have to do anything other than shock absorbers? So we made the world's fanciest shock absorbers, okay? Not just like in your car where there's one layer of them. They're just the right squishiness and so forth. They're better than what's in the cars. And we have four layers of it. So whatever shakes and gets through the first layer, we treat it in a second, third, fourth layer. So it's a mechanical engineering problem. Yeah, that's what I said. So it's not, there's no weird tricks to it, like a chemistry type thing. No, no. Just, well, the right squishiness, you need the right material inside. And ours look like little springs, but they're. Springs? They're springs? So like legitimately, like shock absorbers. Yeah. What? Okay. Okay. And this is now experimental physics at the, at its limit. Okay. So you do this and we make the world's fanciest shock absorbers, just mechanical engineering. Just mechanical engineering, this is hilarious. But we didn't, we weren't good enough to discover gravitational waves. So we did another, we added another feature and it's something else that you're aware of, probably have one. And that is to get rid of noise. You've probably noise, which is, you don't like. And that's the same principle that's in these little Bose earphones. Noise canceling? Noise canceling. So how do they work? They basically, you go on an airplane and they sense the ambient noise from the engines and cancel it. Cause it's just the same over and over again. They cancel it. And when the stewardess comes and asks you whether you want coffee or tea or a drink or something, you hear, you're fine because she's not ambient. She's the signal. So. Are we talking about active canceling? Like where are the. Active canceling. So. This is, okay. So another. Don't tell me you have active canceling on this. Yeah. Besides the shock absorbers. So we had this, so inside this array of shock absorbers. Yeah. We, you asked for some interesting. This is awesome. So inside this, it's harder than the, the earphone problem, but it's just engineering. We have to see measure, not just that the engine still made noise, but the earth is shaking. It's moving in some direction. So we have to actually tell not only that there's noise and cancel it, but what direction it's from. So we put this array of seismometers inside this array of shock absorbers and measure the residual motion and its direction. And we put little actuators that push back against it and cancel it. This is awesome. So you have the actuators and you have the thing that is sensing the, the vibrations and then you have the actual actuators that adjust for that and do so in perfect synchrony. Yeah. What if it all works right. And so how much do we reduce the shaking of the earth? I mean, one part in 10 to the 12th. One part in 10. So what gets through us is one part in 10 to the 12th. That's pretty big reduction. You don't need that in your car, but that's what we do. And so that's how isolated we are from the earth. And that was the biggest, and that was the biggest, I'd say technical problem outside of the physics instrument, the interferometer. Can I ask you a weird question here? You make it very poetically and humorously is saying it's just a mechanical engineering problem, but is this one of the biggest precision mechanical engineering efforts ever? I mean, this seems exceptionally difficult. It is. And so it took a long time. And I think nobody seems to challenge the statement that this is the most precision, precise instrument it's ever been built, LIGO. I wonder what like listening to Led Zeppelin sounds on this thing, because it's so isolated. I mean, this is like, I don't know. No background. No, no back. It's wow. Wow. Wow. So when you were first conceiving this, I would probably, if I was knowledgeable enough, kind of laugh off the possibility that this is even possible. I'm sure, like how many people believe that this is possible? Did you believe this is possible? I did. I didn't know that we needed, for sure that we needed active. When we started, we did dispassive, but we were doing the tests to develop the active to add as a second stage, which we ended up needing. But there was a lot of, you know, now there was a lot of skepticism. A lot of us, especially astronomers, felt that money was being wasted, because we were also expensive. Doing what I told you is not cheap. So it was kind of controversial. It was funded by the National Science Foundation. Can you just linger on this just for a little longer? The actuator thing, the act of canceling. Do you remember like little experiments that were done along the way to prove to the team themselves that this is even possible? Because I work with quite a bit of robots, and to me, the idea that you could do it this precisely is humbling and embarrassing, frankly. Because like, this is another level of precision that I can't even, because robots are a mess. And this is basically one of the most precise robots ever. Right. So like, is there, do you have any like small scale experiments that were done that just be like, this is possible? Yeah, and larger scale. We made a test, that also has to be in vacuum too, but we made test chambers that had this system in it, our first mock of this system, so we could test it and optimize it and make it work. But it's just a mechanical engineering problem. Okay. And humans are just ape descendants. I gotcha. I gotcha. Is there any video of this? Like some kind of educational purpose visualizations of this act of canceling? I don't think so. I mean, does this live on? Well, we work for parts of it, for the active canceling, we worked with, for the instruments, for the sensor and instruments, we worked with a small company near where you are, because it was our MIT people that got them that were, you know, interested in the problem because they thought they might be able to commercialize it for making stable tables to make microelectronics, for example, which are limited by how stable the table is. I mean, at this point, it's a little expensive. So you never know, never know where this leads. So maybe on the, let me ask you, just sticking it a little longer, this silly old mechanical engineering problem. What was to you kind of the darkest moment of what was the hardest stumbling block to get over on the engineer side? Like, was there any time where there's a doubt, where it's like, I'm not sure we would be able to do this, a kind of engineering challenge that was hit? Do you remember anything like that? I think the one that my colleague at MIT, Ray Weiss, worked on so hard and was much more of a worry than this. This is only a question if you're not doing well enough, you have to keep making it better somehow. But this whole huge instrument has to be in vacuum. And the vacuum tanks are, you know, this big around. And so it's the world's biggest high vacuum system. And how do you make it? First of all, how do you make this four meter long sealed vacuum system? It has to be made out of four kilometers, four kilometers long. Would I say something else? Meters. Four kilometers long. Big difference. Yeah. And so, but to make it, yeah, we started with a roll of stainless steel, and then we roll it out like a spiral so that there's a spiral weld on it. Okay, so the engineering was fine. We did that. We worked through very good companies and so forth to build it. But the big worry was, what if you develop a leak? This is a high vacuum, not just vacuum system. Typically, in a laboratory, if there's a leak, you put helium around the thing you have, and then you detect where the helium is coming in. But if you have something as big as this, you can't surround it with helium. So you might not actually even know that there's a leak and it will be affecting it. Well, we can measure how good the vacuum is so we can know that, but a leak can develop and then we don't, how do we fix it or how do we find it? And so that was, you asked about a worry. That was always a really big worry. What's the difference, you know, high vacuum and a vacuum? What is high vacuum? That's like some delta close to vacuum? Is it some threshold? Well, there's a unit. High vacuum is when the vacuum and the units that are used, which are tors, there's 10 to the minus nine. And there's high vacuum is usually used in small places. The biggest vacuum system period is at CERN in this big particle accelerator, but the high vacuum where they need really good vacuum so particles don't scatter in it is smaller than ours. So ours is a really large high vacuum system. I don't know. This is so cool. I mean, this is basically by far the greatest listening device ever built by human. The fact that like descendants of apes could do this, that evolution started with single cell organisms. I mean, is there any more, I'm a huge theory is like, yeah, yeah. But like bridges, when I look at bridges from a civil engineering perspective, it's one of the most beautiful creations by human beings. It's physics. You're using physics to construct objects that can support huge amount of mass and it's like structural, but it's also beautiful. And that humans can collaborate to create that throughout history. And then you take this on another level. This is, this is like, it's exciting to me beyond measure that humans can create something so precise. But another concept lost in this, you just said, you started talking about single cell. Yeah. Okay. You have to realize this discovery that we made that everybody's bought off on happened 1.3 billion years ago, somewhere. And then the signal came to us 1.3 billion years ago, we were just converting on the earth from single cell to multi cell life. So when this actually happened, this collision of two black holes, we weren't here. We weren't even close to developing single. Yeah, we were had, we're going from single cell to multi cell life at that point. All to meet up at this, at this point. Yeah. Wow. That's like, that's almost romantic. It is. Okay. So on the human side of things, it's kind of fascinating because you're talking about over a thousand people team for LIGO. Yeah. They started out with, you know, around a hundred and you've for parts of the time at least led this team. What does it take to lead a team like this of incredibly brilliant theoreticians and engineers and just a lot of different parties involved? A lot of egos, a lot of ideas. You had this fun, funny example, I forget where, where in publishing a paper, you have to all agree on like, you know, the phrasing of a certain sentence or the title of the paper and so on. That's a very interesting, simple example. I'd love you to speak to that, but just in general, how, what does it take to lead this kind of team? Okay. I think that the general idea is one we all know. You want to, you want to, you want to get where the, the sum of something is more than the individual parts is what we say, right? Yeah. So that's what you're trying to achieve. Yes. Okay. How do you do that? Actually, mostly if we take multiple objects or people, I mean, you put them together, the sum is less. Yes. Why? Because they overlap. So you don't have individual things that, you know, this person does that, this person does that, then you get exactly the sum. But what you want is to develop where you get more than what the individual contributions are. We know that's very common. People use that expression everywhere. And it's the expression that has to be kind of built into how people feel it's working. Because if you're part of a team, and you realize that somehow the team is able to do more than the individuals could do themselves, then they buy on kind of in terms of the process. So that's the, that's the goal that you have to have is to, to achieve that. And that means that you have to realize parts of what you're trying to do that require not that one person couldn't do it, it requires the combined talents to be able to do something that neither of them could do themselves. And we have a lot of that kind of thing. And I think, I mean, build into the some of the examples that I gave you. And so, how do you then, so, so the key almost in anything you do is the people themselves, right? So in our case, the first and most important was to attract to spend years of their life on this. And the best possible people in the world to do it. So the only way to convince them is that somehow it's better and more interesting for them than what they could do themselves. And so that's part of this idea. Yeah, that's powerful. But nevertheless, there's best people in the world, there's egos. Is there something to be said about managing egos? Oh, that's the human problem is always the hardest. And so there's, that's an art, not a science, I think. I think the fact here that combined, there's a was a romantic goal that we had to, you know, do something that people hadn't done before, which was important scientifically and, and a huge challenge, enabled us to say, take and get, I mean, what we did just to take an example, we use the light to go in this thing comes from lasers. We need a certain kind of laser. So the kind of laser that we use, there were three different institutions in the world that had the experts that do this, maybe in competition with each other. So we got all three to join together and work with us to work on this as an example. So that you had, and they had the thing that they were working together on a kind of object that they wouldn't have otherwise. And we're part of a bigger team where they could discover something that isn't even engineers. These are engineers that do laser. So, and they're part of our laser physicists. So could you describe the moment or the period of time when finally this incredible creation of human beings led to a detection of gravitational waves? It's a long story. Unfortunately, this is a part that we started failures along the way kind of thing or all failures. That's all that's built into it. If you're not, if you're not mechanical engineering, you build on your failures, that's expected. So we're trying things that no one's done before. So it's technically not just gravitational waves. And so it's built on failures. But anyway, we did before me, even there, the people did R&D on the concepts. But starting in 1994, we got money from the National Science Foundation to build this thing. It took about five years to build it. So by 1999, we had built the basic unit. It did not have active seismic isolation at that stage, didn't have some other things that we have now. What we did at the beginning was stick to technologies that we had at least enough knowledge that we could make work or had tested in our own laboratories. And so then we put together the instrument. We made it work. It didn't work very well, but it worked. And we didn't see any gravitational waves. Then we figured out what limited us. And we went through this every year for almost 10 years, never seeing gravitational waves. We would run it, looking for gravitational waves for months, learn what limited us, fix it for months, and then run it again. Eventually, we knew we had to take another big step. And that's when we made several changes, including adding these active seismic isolation, which turned out to be a key. And we fortunately got the National Science Foundation to give us another couple hundred million dollars, 100 million more. And we rebuild it or fixed or improved it. And then in 2015, we turned it on. And we almost instantly saw this first collision of two black holes. And then we went through a process of, do we believe what we've seen? Yeah, I think you're one of the people that went through that process. It sounds like some people immediately believed it. And then you're like... So as human beings, we all have different reactions to almost anything. And so quite a few of my colleagues had a eureka moment immediately. I mean, the figure that we put in our paper, first is just data. We didn't have to go through fancy computer programs to do anything. And we show next to it the calculations of Einstein's equations. It looks just like what we detected. And we did it in two different detectors halfway across the US. So it was pretty convincing, but you don't want to fool yourself. So being a scientist, for me, we had to go through and try to understand that the instrument itself, which was new, I said we had rebuild it, couldn't somehow generate things that look like this. That took some tests. And then the second, you'll appreciate more, we had to somehow convince ourselves we weren't hacked in some clever way. Cybersecurity question. Yeah. Even though we're not on the internet, but... Yeah. No, it can be physical access too. Yeah. That's fascinating. It's fascinating that you would think about that. I mean, not enough. I mean, because it matches prediction. So the chances of it actually being manipulated is very, very low. But nevertheless... We still could have disgruntled all the graduate students who had worked with us earlier that... Who want you to... I don't know how that's supposed to embarrass you. I suppose, yeah. I suppose I see. But about what I think you said, within a month, you kind of convinced yourself officially. Within a month, we convinced ourselves. We kept a thousand collaborators quiet during that time. Then we spent another month or so trying to understand what we'd seen so that we could do the science with it instead of just putting it out to the world and let somebody else understand that it was two black holes and what it was. The fact that a thousand collaborators were quiet is a really strong indication that this is a really close knit team. Yeah. And they're around the world. Either strong knit or tight knit or had a strong dictatorship or something. Yeah. Either fear or love. You can rule by fear or love. Yeah, right. You can go back to Machiavelli. Yeah. All right. Well, this is really exciting that that's a success story because it didn't have to be a success story, right? I mean, eventually, perhaps you could say it'll be an event, but it could have taken over a century to get there. Oh, yeah. Yeah. And it's only downhill now. What do you mean? You mean with gravitational waves? Yeah. Well, now we're off because of the pandemic, but when we turned off, we were seeing some sort of gravitational wave event each week. Now we're fixing, we're adding features where it'll probably be when we turn back on next year, it'll probably be one every couple days. And they're not all the same. So it's learning about what's out there in gravity instead of just optics. So it's all great. We're only limited by the fantastic thing other than that this is a great field and it's all new and so forth is that experimentally, the great thing is that we're limited by technology and technical limitations, not by science. So another really important discovery that was made before ours was what's called the Higgs boson made on the big accelerator at CERN. This huge accelerator, they discovered a really important thing. We have Einstein's equation, E equals MC squared. So energy makes mass or mass can make energy and that's the bomb. But the mechanism by which that happens, not vision, but how do you create mass from energy was never understood until there was a theory of it about 70 years ago now. And so they discovered it's named after a man named Higgs. It's called the Higgs boson. And so it was discovered, but since that time, and I worked on those experiments since that time, they haven't been able to progress very much further, a little bit, but not a lot further. And the difference is that we're really lucky we're in what we're doing in that there you see this Higgs boson, but there's tremendous amount of other physics that goes on and you have to pick out the needle in the haystack of physics. You can't make the physics go away, it's there. In our case, we have a very weak signal, but once we get good enough to see it, it's weak compared to where we've reduced the background, but the background is not physics, it's just technology. It's getting ourselves better isolated from the Earth or getting a more powerful laser. And so since 2015, when we saw the first one, we continually can make improvements that are enabling us to turn this into a real science to do astronomy, a new kind of astronomy. It's a little like astronomy. Galileo started the field. He basically took lenses that were made for classes and he didn't invent the first telescope, but made a telescope, looked at Neptune and saw that it had four moons. That was the birth of not just using your eyes to understand what's out there. And since that time, we've made better and better telescopes, obviously, and astronomy thrives. And in a similar way, we're starting to be able to crawl, but we're starting to be able to do that with gravitational waves. And it's going to be more and more that we can do as we can make better and better instruments because, as I say, it's not limited by picking it out of others. Yeah, it's not limited by the physics. So you have an optimism about engineering that as human progress marches on, engineering will always find a way to build a large enough device, accurate enough device to detect the same thing. As long as it's not limited by physics, yeah, they'll do it. So you, two other folks and the entire team won the Nobel prize for this big effort. There's a million questions I can ask for, but looking back, where does the Nobel prize fit into all of this? If you think hundreds of years from now, I venture to say that people will not remember the winners of a prize, but they'll remember creations like these. Maybe I'm romanticizing engineering, but I guess I want to ask how important is the Nobel prize in all of this? Well, that's a complicated question. As a physicist, it's something if you're trying to win a Nobel prize, forget it because they give one a year. So there's been 200 physicists who have won the Nobel prize since 1900. And so things just have to fall right. So your goal cannot be to win a Nobel prize. It wasn't my dream. It's tremendous for science. Why the Nobel prize for a guy that made dynamite and stuff is what it is. It's a long story, but it's the one day a year where actually the science that people have done is all over the world and so forth. Forget about the people again. It is really good for science. It celebrates science for several days, different fields, chemistry, medicine and so forth. And everybody doesn't understand everything about these. They're generally fairly abstract, but then it's on the front page of newspapers around the world. So it's really good for science. It's not easy to get science on the front page of the New York Times. It's not there. Should be, but it's not. And so the Nobel prize is important in that way. Otherwise, I have a certain celebrity that I didn't have before. And now you get to be a celebrity that advertises science. It's a mechanism to remind us how incredible, how much credit science deserves and everything. Well, it has a little bit more. One thing I didn't expect, which is good, is that we have a government. I'm not picking on ours necessarily, but it's true of all governments are not run by scientists. In our case, it's run by lawyers and businessmen. Yep. Okay. And at best they may have an aide or something that knows a little science. So in all countries hardly take into account science in making decisions. Yes. Okay. And having a Nobel prize, the people in those positions actually listen. So you have more influence. I don't care whether it's about global warming or what the issue is. There's some influence, which is lacking otherwise. And people pay attention to what I say. If I talk about global warming, they wouldn't have before I had the Nobel prize. Yeah, this is very true. You're like the celebrities who talk. Celebrity has power. Celebrity has power. And that's a good thing. That's a good thing. Singling out people, I mean, on the other side of it, singling out people has all kinds of, whether it's for Academy Awards or for this, have unfairness and arbitrariness and so forth and so on. So that's the other side of the coin. Just like you said, especially with the huge experimental projects like this, you know, it's a large team and it does the nature of the Nobel prizes. It singles out a few individuals to represent the team. Yeah. Nevertheless, it's a beautiful thing. What are ways to improve LIGO in the future, increase the sensitivity? I've seen a few ideas that are kind of fascinating. Are you interested in them? I'm not speaking about five years. Perhaps you could speak to the next five years, but also the next hundred years. Yeah. So let me talk to both the instrument and the science. Sure. So they go hand in hand. I mean, the thing that I said is if we make it better, we see more kinds of weaker objects and we do astronomy. Okay. We're very motivated to make a new instrument, which will be a big step, the next step, like making a new kind of telescope or something. And the ideas of what that instrument should be haven't converged yet. There's different ideas in Europe. They've done more work to kind of develop the ideas, but they're different from ours and we have ideas. But I think over the next few years, we'll develop those. The idea is to make an instrument that's at least 10 times better than what we can do with this instrument, 10 times better than that. 10 times better means you can look 10 times further out. 10 times further out is a thousand times more volume. So you're seeing much, much more of the universe. The best way to look at it is to look further out. The big change is that if you can see far out, you see further back in history. Yeah, you're traveling back in time. Yeah. And so we can start to do what we call cosmology instead of astronomy or astrophysics. Cosmology is really the study of the evolution of the universe. And so then you can start to hope to get to the important problems having to do with how the universe began, how it evolved and so forth, which we really only study now with optical instruments or electromagnetic waves. And early in the universe, those were blocked because it was, basically it wasn't transparent. So the photons couldn't get out when everything was too dense. What do you think, sorry on this tangent, what do you think an understanding of gravitational waves from earlier in the universe can help us understand about the Big Bang and all that kind of stuff? Yeah. But it's a non, it's another perspective on the thing. Is there some insights you think could be revealed just to help a layman understand? Sure. First, we don't understand. We use the word Big Bang. We don't understand the physics of what the Big Bang itself was. So I think, and in the early stage, there were particles and there was a huge amount of gravity and mass being made. So I'll say two things. One is, how did it all start? How did it happen? I'll give you at least one example that we don't understand what we should understand. We don't know why we're here. Yes. No, we do not. I don't mean it philosophically. I mean it in terms of physics. Now, what do I mean by that? If I go into my laboratory at CERN or somewhere and I collide particles together or put energy together, I make as much anti matter as matter. Anti matter then annihilates matter and makes energy. So in the early universe, you made somehow a lot of matter and anti matter, but there was an asymmetry. Somehow there was more matter and anti matter. The matter and anti matter annihilated each other. At least that's what we think. And there was only matter leftover. And we live in a universe that we see this all matter. We don't have any idea. We have ideas, but we don't have any way to understand that at the present time with the physics that we know. Can I ask a dumb question? Does anti matter have anything like a gravitational field to send signals? So how does this asymmetry of matter and anti matter could be investigated or further understood by observing gravitational fields or weirdnesses in gravitational fields? I think that in principle, if there were anti neutron stars, instead of just neutron stars, we would see different kinds of signals, but it didn't get to that. We live in a universe that we've done enough looking because we don't see anti matter, anti protons anywhere, no matter what we look at, that it's all made out of matter. Hmm. There is no anti matter except when we go in our laboratories. So, but when we go in our laboratories, we make as much anti matter as matter. So there's something about the early universe that made this asymmetry. So we can't even explain why we're here. That's what I meant. Physics wise, not in terms of how we evolved and all that kind of stuff. So there might be inklings of some of the physics that gravitational So gravitational waves don't get obstructed like light. So I said light only goes to 300,000 years. So it goes back to the beginning. So if you could study the early universe with gravitational waves, we can't do that yet. Then it took 400 years to be able to do that with optical, but but then you can really understand the very, maybe understand the very early universe. So in terms of questions like why we're here or what the big bang was, we should be, we can, in principle, study that with gravitational waves. So to keep moving in this direction, it's a unique kind of way to understand our universe. So you think there's more Nobel prize level ideas to be discovered in relation to I'd be shocked if there, if there isn't, not even going to that, which is a very long range problem. But I think that we only see with electromagnetic waves, 4% of what's out there. There must be, we looked for things that we knew should be there. There should be, I would be shocked if there wasn't physics, objects, science, and with gravity that doesn't show up in everything we do with telescopes. So I think we're just limited by not having powerful enough instruments yet to do this. Do you have a preference? I keep seeing this E. Lisa idea. Yeah. Is it, do you have a preference for earthbound or space faring mechanisms for? They're complimentary. It's a little bit like, it's completely analogous to what's been done in astronomy. So astronomy from the time of Galileo was done with visible light. The big advances in astronomy in the last 50 years are because we have instruments that look at the infrared, microwave, ultraviolet and so forth. So looking at different wavelengths has been important. Basically going into space means that we'll look at instead of the audio band, which we look at, as we said on the Earth's surface, we'll look at lower frequencies. So it's completely complimentary and it starts to be looking at different frequencies just like we do with astronomy. It seems almost incredible to me, engineering wise, just like on earth to send something that's kilometers across into space. Is that harder to engineer? It actually is a little different. It's three satellites separated by hundreds of thousands of kilometers and they send a laser beam from one to the other. And if the triangle changes shape a little bit, they detect that from a graph. Did you say hundreds of thousands of kilometers? Yeah. Sending lasers to each other. Okay. It's just engineering. Is it possible though? Is it doable? Yes. Okay. That's just incredible because they have to maintain, I mean, the precision here is probably, there might be some more, what is it? Maybe noise is a smaller problem. I guess there's no vibration to worry about like seismic stuff. So getting away from earth, maybe you get away from seismic stuff. Yeah. Those parts are easier. They don't have to measure it as accurately at low frequencies. But they have a lot of tough engineering problems. In order to detect that the gravitational waves affect things, the sensors have to be what we call free masses, just like ours, are isolated from the earth. They have to isolate it from the satellite. And that's a hard problem. They have to do that pretty, not as well as we have to do it, but very well. And they've done a test mission and the engineering seems to be at least in principle in hand. This will be in the 2030s. 2030s? Yeah. This is incredible. This is incredible. Let me ask about black holes. So what we're talking about is observing orbiting black holes. I saw the terminology of like binary black hole systems. Binary black holes. Is that the one that's when they're dancing? Okay. They're both going around each other, just like the earth around the sun. Okay. Is that weird that there's black holes going around each other? So the finding binary systems of stars is similar to finding binary systems of... Of black holes. Well, they were once stars. So we haven't said what a black hole is physically yet. Yeah. What's a black hole? So black hole is first, it's a mathematical concept or a physical concept. And that is a region of space. So it's simply a region of space where the curvature of space time, meaning the gravitational field is so strong that nothing can get out, including light. And there's light gets bent if the space time is warped enough. And so even light gets bent around and stays in it. So that's the concept of a black hole. And maybe you can make... So that's a concept that didn't say how they come about. And there could be different ways they come about. The ones that we are seeing, we're not sure. That's what we're trying to learn now is what they... But the general expectation is that they come... These black holes happen when a star dies. So what does that mean that a star dies? What happens? A star like our sun basically makes heat and light by fusion. It's made up. And as it burns, it burns up the hydrogen and then the helium and slowly works its way up to the heavier and heavier elements that are in the star. And when it gets up to iron, the fusion process doesn't work anymore. And so the stars die and that happens to stars. And then they do what's called a supernova. What happens then is that a star is a delicate balance between an outward pressure from fusion and light and burning and an inward pressure of gravity trying to pull the masses together. Once it burns itself out, it goes and it collapses and that's a supernova. When it collapses, all the mass that was there is in a very much smaller space. And if a star, if you do the calculations, if a star is big enough, that can create a strong enough gravitational field to make a black hole. Our sun won't. It's too small. Too small. And we don't know exactly what, but it's usually thought that a star has to be at least three times as big as our sun to make a black hole. But that's the physical way there. You can make black holes. That's the first explanation that one would give for what we see, but it's not necessarily true. We're not sure yet. What we see in terms of, for the origins of black holes? No, the black holes that we see in gravitational waves. So the, but you're also looking for the ones who are binary solar systems. So they're binary systems, but they could have been made from binary stars. So there's binary stars around. So that's, so that's the first explanation is that that's what they are. Gotcha. Other explanations, but what we see has some puzzles. This is kind of the way science works, I guess. We see heavier ones than up to, we've seen one system that was 140 times the mass of our own sun. That's not believed to be possible with the parent being a big star because big stars can only be so big or they are unstable. It's just the fact that they live in an environment that makes them unstable. So the fact that we see bigger ones, they may be come from something else. It's possible that they were made in a different way by little ones eating each other up or maybe they were made or maybe they came with the big bang. The prime, what we call primordial, which means they're really different. They came from that. We don't know at this point if they came with a big bang, then maybe they account for what we call dark matter or some of it. Hmm. Like there was a lot of them if they came with it because there's a lot of dark matter. Yeah. But will gravitational waves give you any kind of intuition about the origin of these oscillating? We think that if we see the distributions enough of them, the distributions of their masses, the distributions of how they're spinning, so we can actually measure when they're going around each other, whether they're spinning like this or whether the whole system has any wobbles. What? So this is now. Okay. We're doing that. And then you're constantly kind of crawling back and back in time. And we're crawling back in time and seeing how many there are as we go back. And so do they point back. So you're like, what is that discipline called, cartography or something? You're like mapping this, the early universe via the lens of gravitational waves. Not yet the early universe, but at least back in time. Earlier. Yeah. So black holes are this mathematical phenomenon, but they come about in different ways. We have a huge black hole at the center of our galaxy and other galaxies. Those probably were made some other way. We don't know when the galaxies themselves had to do with the formation of galaxies. We don't really know. So the fact that we use the word black hole, the origin of black holes might be quite different depending on how they happen. They just have to in the end have a gravitational field that will bend everything in. How do you feel about black holes as a human being? There's this thing that's nearly infinitely dense, doesn't let light escape. Isn't that kind of terrifying? It feels like the stuff in nightmares. I think it's an opportunity. To do what exactly? So like the early universe is an opportunity. If we can study the early universe, we can learn things like I told you. And here again, we have an embarrassing situation in physics. We have two wonderful theories of physics, one based on quantum mechanics, quantum field theory. And we can go to a big accelerator like at CERN and smash particles together and almost explain anything that happens beautifully using quantum field theory and quantum mechanics. Then we have another theory of physics called general relativity, which is what we've been talking about most of the time, which is fantastic at describing the things at high velocities, long distances, and so forth. So that's not the way it's supposed to be. We're trying to create a theory of physics, not two theories of physics. So we have an embarrassment that we have two different theories of physics. People have tried to make a unified theory, what they call a unified theory. You've heard those words for decades. They still haven't. That's been primarily done theoretically or tried. People actively do that. My personal belief is that like much of physics, we need some clues. So we need some experimental evidence. So where is there a place? If we go to CERN and do those experiments, gravitational waves or general relativity don't matter. If we go to study our black holes, elementary particle physics doesn't matter. We're studying these huge objects. So where might we have a place where both phenomena have to be satisfied? An example is black holes. Inside black holes. Yeah. So we can't do that today. But when I think of black hole, it's a potential treasure chest of understanding the fundamental problems of physics and maybe can give us clues to how we bring to the embarrassment of having two theories of physics together. That's my own romantic idea. What's the worst that could happen? It's so enticing. Just go in and look. Do you think, how far are we away from figuring out the unified theory of physics, the theory of everything? What's your sense? Who will solve it? Like what discipline will solve it? Yeah. I think so little progress has been made without more experimental clues, as I said, that we're just not able to say that we're close without some clues. The most popular theory these days that might lead to that is called string theory. The problem with string theory is it solves a lot of beautiful mathematical problems we have in physics. It's very satisfying theoretically, but it has almost no predictive, maybe no predictive ability because it is a theory that works in 11 dimensions. We live in a physical world of three space and one time dimension. In order to make predictions in our world with string theory, you have to somehow get rid of these other seven dimensions. That's done mathematically by saying they curl up on each other on scales that are too small to affect anything here. That's an okay argument, but how you do that is not unique. That means if I start with that theory and I go to our world here, I can't uniquely go to it. And if I can't, it's not predictive. And that's actually a killer. That's a killer. And string theory is, it seems like from my outsider's perspective has lost favor over the years, perhaps because of this very idea. It's a lack of predictive power. I mean, that science has to connect to something where you make predictions as beautiful as it might be. So I don't think we're close. I think we need some experimental clues. It may be that information on something we don't understand presently at all, like dark energy or probably not dark matter, but dark energy or something might give us some ideas. But I can't envision right now in the short term, meaning the horizon that we can see how we're going to bring these two theories together. A kind of a two part question, maybe just asking the same thing in two different ways. One question is, do you have hope that humans will colonize the galaxy? So expand out, become a multi planetary species. Another way of asking that from a gravitational and a propulsion perspective, do you think we'll come up with ways to travel closer to the speed of light or maybe faster than the speed of light, which would make it a whole heck of a lot easier to expand out into the universe? Yeah. Well, I think that's very futuristic. I think we're not that far from being able to make a one way trip to Mars. That's then a question of whether people are willing to send somebody on a one way trip. Oh, I think they are. There's a lot of the explorers burned bright within our hearts. Yeah, exactly. There's a lot of people willing to die for the opportunity to explore new territory. So this recent landing on Mars is pretty impressive. They have a little helicopter. They're going to fly around. You can imagine in the not too distant future that you could have, I don't think civilizations colonizing, I can envision, but I can envision something more like the South Pole. We haven't colonized Antarctica because it's all ice and cold and so forth. But we have stations. So we have a station that's self sustaining at the South Pole. I've been there. It has. Wow, really? Yeah. What's that like? Because there's parallels there to go to Mars. It's fantastic. What's the journey like? The journey involves going. The South Pole station is run in the US by the National Science Foundation. I went because I was on the National Science Board that runs the National Science Foundation. And so you get a VIP trip if you're healthy enough to the South Pole to see it, which I took. You fly from the US to Australia to Christchurch in Southern Australia. And from there you fly to McMurdo Station, which is on the coast. And it's the station with about a thousand people right on the coast of Antarctica. It's about a seven or eight hour flight and they can't predict the weather. So when I flew from Christchurch to McMurdo Station, they tell you in advance, you do it in a military aircraft, they tell you in advance that they can't predict whether they can land because they have to land on ice. And reassuring. Yeah. And so about halfway the pilot got on and said, sorry, this is a, they call it a boomerang flight. You know, boomerang goes out and goes back. So we had to stay a little while in Christchurch, but then we eventually went to McMurdo Station and then flew to the South Pole. The South Pole itself is, when I was there, it was minus 51 degrees. That was summer. Zero humidity. And it's about 11,000 feet altitude because it's never warm enough for anything to melt. So it doesn't snow very much, but it's about 11,000 feet of snowpack. So you land in a place that's high altitude, cold as could be, and incredibly dry, which means you have a physical adjustment. The place itself is fantastic. They have this great station there. They do astronomy at the South Pole. Nature wise, is it beautiful? What's the experience like? Or is it like visiting any town? No, it's very small. There's only less than a hundred people there. Even when I was there, there were about 50 or 60 there. And in the winter, there's less, half of that. Their winter. Yeah. It gets real cold. It gets really cold, yeah. But it's a station. And I think, and that's, I mean, we haven't gone beyond that. On the coast of Antarctica, they have greenhouses and they're self sustaining in McMurdo Station, but we haven't really settled more than that kind of thing in Antarctica, which is a big country or a big plot, a big piece of land. So I don't, I can't envision kind of colonizing at people living so much, as much as I can see the equivalent There's people that engineer viruses to protect us from viruses to see how close is this to mutating so it can jump to humans or engineering defenses against those. And it seems exciting and the application, the positive applications are really exciting at this time, but we don't think about how that runs away in decades to come. Yeah. And I think it's the same idea as this little book, The Ratchet of Science, The Ratchet of Curiosity. I mean, whether you pursue, take curiosity and let artificial intelligence or machine learning run away with having its solutions to whatever you want, or we do it, it's, I think, a similar consequence. I think from what I've read about Enrico Fermi, he became a little bit cynical about the human species towards the end of his life, both having observed what he observed. Well, he didn't write much. I mean, he died young. He died soon after the World War. There was already, you know, the work by Teller to develop the hydrogen bomb. And I think he was a little cynical of that, you know, pushing it even further and rising tensions between the Soviet Union and the U.S. and looked like an endless thing. So, but he didn't say very much, but a little bit, as you said. Yeah, there's a few clips to sort of maybe picked on a bad mood, but in a sense that almost like a sadness, a melancholy sadness to a hope that waned a little bit about that perhaps we can do, like this curious species can find the way out. Well, especially, I think, people who worked like he did at Los Alamos and spent years of their life somehow had to convince themselves that dropping these bombs would bring lasting peace and that it didn't. Yeah. As a small, interesting aside, it'd be interesting to hear if you have opinions on this. His name is also attached to the Fermi Paradox, which asks if there is a, you know, it's a very interesting question, which is if it does seem if you sort of reason basically that there should be a lot of alien civilizations out there. If the human species, if Earth is not that unique by basic, no matter the values you pick, it's likely that there's a lot of alien civilizations out there. And if that's the case, why have they not at least obviously visited us or sent us loud signals that everybody can hear? Fermi's quoted as saying, sitting down at lunch, I think it was with Teller and Herb York, who was kind of one of the fathers of the atomic bomb. And he sat down and he said something like, where are they? Which meant, where are these other? And then he did some numerology where he calculated, you know, how many, what they knew about how many galaxies there are and how many stars and how many planets then are like the Earth and blah, blah, blah. That's been done much better by somebody named Drake. And so, people usually refer to the, I don't know whether it's called the Drake formula or something, but it has the same conclusion. The conclusion is it would be a miracle if there weren't other, you know, the statistics are so high that how can we be singular and separate? So, probably there is, but there's almost certainly life somewhere. Maybe there was even life on Mars a while back, but intelligent life, probably. So, you know, the statistics say that communicating with us, I think that it's harder than people think. We might not know the right way to expect the communication, but all the communication that we know about travels at the speed of light. And we don't think anything can go faster than the speed of light. That limits the problem quite a bit. And it makes it difficult to have any back and forth communication. You could send signals like we try to or look for, but to have any communication, it's pretty hard when it has to be close enough that the speed of light would mean we could communicate with each other. And I think, and we didn't even understand that. I mean, we're an advanced civilization, but we didn't even understand that a little more than a hundred years ago. So, are we just not advanced enough? Maybe to know something about that's the speed of light. Maybe there's some other way to communicate that isn't based on electromagnetism. I don't know. Gravity seems to be also have the same speed. That was a principle that Einstein had and something we've measured actually. So is it possible? I mean, so we'll talk about gravitational waves and in some sense, there's a brainstorming going on, which is like, how do we detect the signal? Like what would a signal look like and how would we detect it? And that's true for gravitational waves. That's true for basically any physics phenomena. You have to predict that that signal should exist. You have to have some kind of theory and model why that signal should exist. I mean, is it possible that aliens are communicating with us via gravity? Like why not? Well, yeah, it's true. Why not? For us, it's very hard to detect these gravitational effects. They have to come from something pretty that has a lot of gravity like black holes, but we're pretty primitive at this stage. There's very reputable physicists that look for a fifth force, one that we haven't found yet. Maybe it's the key. What would a fifth force of physics look like exactly? Well, usually they think it's probably a longer range force than we have now. But there are reputable colleagues of mine that spend their life looking for a fifth force. So longer range than gravity? Yeah. Super long? It doesn't fall off like one over r squared, but maybe separately. Gravity, Newton taught us, goes like inversely one over the square of the distance apart you are. So it falls pretty fast. That's okay. So now we have a theory of what consciousness is. It's just the fifth force of physics. Yeah. There we go. That's a good hypothesis. Speaking of gravity, what are gravitational waves? Let's maybe start from the basics. We learned gravity from Newton, right? When you were young, you were told that if you jumped up, the earth pulls you down. And when the apple falls out of the tree, the earth pulls it down. And maybe you even asked your teacher why, but most of us accepted that. That was Newton's picture, the apple falling out of the tree. But Newton's theory never told you why the apple was attracted to the earth. That was a missing in Newton's theory. Newton's theory also Newton recognized at least one of the two problems. I'll tell you one of them is there's more than those, but one is why does the earth, what's the mechanism by which the earth pulls the apple or holds the moon when it goes around, whatever it is. That's not explained by Newton, even though he has the most successful theory of physics ever went 200 and some years with nobody ever seeing a violation. But he accurately describes the movement of an object falling down to earth, but he's not answering why that what's yeah, because it's a distance. He gives a formula, which it's a product of the earth's mass, the apple's mass inversely proportional to the square of the distance between and then the strength he called capital G, the strength he couldn't determine, but it was determined 100 years later. But no one ever saw a violation of this until a possible violation, which Einstein fixed, which was very small that has to do with mercury going around the sun, the orbit being slightly wrong if you calculate it by Newton's theory. But so like most theories then in physics, you can have a wonderful one like Newton's theory. It isn't wrong. But you have to have an improvement on it to answer things that it can't answer. And in this case, Einstein's theory is the next step. We don't know if it's anything like a final theory or even the only way to formulate it either. But he formulated this theory, which he released in 1915. He took 10 years to develop it, even though in 1905, he solved three or four of the most important problems in physics in a matter of months. And then he spent 10 years on this problem before he of the South Pole Station. Well, in the computing world, there's an idea of backing up your data and then you want to do offsite backup, to make sure that if the whole thing burns, if your whole house burns down, that you can have a backup offsite of the data. I think the difference between Antarctica and Mars is Mars is an offsite backup. That if we have nuclear war, whatever the heck might happen here on earth, it'd be nice to have a backup elsewhere. And it'd be nice to have a large enough colony where we sent a variety of people except a few silly astronauts in suits, have an actual vibrant, get a few musicians and artists up there, get a few, maybe like one or two computer scientists, those are essential. Maybe even a physicist, but I'm not sure. Yeah, maybe not. So that comes back to something you talked about earlier, which is the paradox, Fermi's paradox, because you talked about having to escape. And so one number you don't know how to use in Fermi's calculation or Drake, who's done it better, is how long do civilizations last? We've barely gotten to where we can communicate with electricity and magnetism and maybe we'll wipe ourselves out pretty soon. Are you hopeful in general? Like you think we've got another couple of hundred years at least? Or are you worried? Well, no, I'm hopeful, but I don't know if I'm hopeful in the longterm. If you say, are we able to go for another couple of thousand years? I'm not sure. I think we have where we started, the fact that we can do things that don't allow us to kind of keep going or there can be, whether it ends up being a virus that we create or ends up being the equivalent of nuclear war or something else. It's not clear that we can control things well enough. So speaking of really cold conditions and not being hopeful and eventual suffering and destruction of the human species, let me ask you about Russian literature. You mentioned, how's that for transition? I'm doing my best here. You mentioned that you used to love literature when you were younger and you even were hoping to be a writer yourself. That was the motivation. And some of the books I've seen that you listed that were inspiring to you was from Russian literature, like Tolstoy, Dostoevsky, Solzhenitsyn. Maybe in general you can speak to your fascination with Russian literature or in general what you picked up from those. I'm not surprised you picked up on the Russian literature, your background, but that's okay. You should be surprised I didn't make the entire conversation about this. That's the real surprise. Yeah. When I didn't really become a physicist or want to go in science until I started college. So when I was younger, I was good at math and that kind of stuff, but I didn't really, I came from a family, nobody went to college and I didn't have any mentors. But I liked to read when I was really young. And so when I was very young, I always carried around a pocket book and read it. And my mother read these mystery stories and I got bored by those eventually. And then I discovered real literature. I don't know what age, but about 12 or 13. And so then I started reading good literature and there's nothing better than Russian literature, of course. Thank you. Reading good literature. So I read quite a bit of Russian literature at that time. And so you asked me about, well, I don't know, I'll say a few words, Dostoevsky. So what about Dostoevsky? For me, Dostoevsky was important in two, I mean, I've read a lot of literature because it's kind of the other thing I do with my life. And he made two incredible, in addition to his own literature, he influenced literature tremendously by having, I don't know how to pronounce polyphony. So he's the first real serious author that had multiple narrators. And he absolutely is the first. And he also was the first, he began existential literature. So the most important book that I've read in the last year when I've been forced to be isolated was existential literature. I decided to reread Camus, The Plague. Oh, yeah. That's a great book. It's a great book and it's right now to read it. It's fantastic. I think that book is about love, actually. Love for humanity. It is, but it has all the, if you haven't read it in recent years, I had read it before, of course, but to read it during this, because it's about a plague. So it's really fantastic to read down. But that reminds me of, he was a great existentialist, but the beginning of existential literature was Dostoevsky. Dostoevsky, yeah. So in addition to his own great novels, he had a tremendous impact on literature. And there's also for Dostoevsky, unlike most other existentialists, he was at least in part religious. I mean, religiosity permeated his idea. I mean, one of my favorite books of his is The Idiot, which is a Christlike figure in there. Well, there's Prince Mishkin, is that his name? Prince Mishkin, yeah. Yeah, Mishkin. Yeah, Mishkin. Yeah. That's one thing about, you read it in English, I presume. Yeah, yeah. Yeah. So the names, that's what gets a lot of people. There's so many names, so hard to pronounce. You have to remember all of them. It's like you have the same problem. But he was a great character. I kind of have a connection with him, because I often, the title of the book, The Idiot, is I kind of, I often call myself an idiot, because that's how I feel. I feel so naive about this world. And I'm not sure, I'm not sure why that is. Maybe it's genetic or so on. But I have a connection, a spiritual connection to that character. To Mishkin. To Mishkin, yeah. But he was far from an idiot. No, in some sense, in some sense. But in another sense, maybe not of this world. In another sense he was. I mean, he was a bumbler, a bunker. But you also mentioned Solzhenitsyn, very interesting. And he always confused me. Of course, he was really, really important in writing about Stalin, and first getting in trouble, and then later he wrote about Stalin in a way, I forget what the book was, in a way that was very critical of Lenin. Yeah, he's evolved through the years, and he actually showed support for Putin eventually. It was a very interesting transition he took, no, journey he took through thinking about Russia and the Soviet Union. But I think what I get from him is basic, it's like Viktor has this man's search for meaning. I have a similar kind of sense of the cruelty of human nature, cruelty of indifference, but also the ability to find happiness in the small joys of life. That's something, there's nothing like a prison camp that makes you realize you could still be happy with a very, very little. Yeah, his description of how to go through a day and actually enjoy it in a prison camp is pretty amazing. And some prison camp, it's the worst of the worst. And also, I do think about the role of authoritarian states in hopeful idealistic systems somehow leading to the suffering of millions. And this might be arguable, but I think a lot of people believe that Stalin, I think, genuinely believed that he's doing good for the world. And he wasn't. It's a very valuable lesson that even evil people think they're doing good. Otherwise, it's too difficult to do the evil. The best way to do evil is to believe about framing it in a way like you're doing good. And then this is a very clear picture of that, which is the gulags. And Solzhenitsyn is one of the best people to reveal that. The most recent thing I read, it isn't actually fiction, was the woman, I can't remember her name, who got the Nobel Prize about within the last five years. I don't know whether she's Ukrainian or Russian, but there are interviews. Have you read that? Interview of Ukrainian survivors of... Well, I think she may be originally Ukrainian. The book's written in Russian and translated in English, and many of the interviews are in Moscow and places. But she won the Nobel Prize within the last five years or so. But what's interesting is that these are people of all different ages, all different occupations and so forth, and they're reflecting on their reaction to basically the present Soviet system, the system they lived with before. There's a lot of looking back by a lot of them with, well, it being much better before. Yeah. I don't know what... In America, we think we know the right answer, what it means to be, to build a better world. I'm not so sure. I think we're all just trying to figure it out. Yeah, there's... We're doing our best. I think you're right. Is there advice you can give to young people today, besides reading Russian literature at a young age, about how to find their way in life, how to find success in Korea or just life in general? My own belief, it may not be very deep, but I believe it. I think you should follow your dreams and you should have dreams and follow your dreams if you can, to the extent that you can. And we spend a lot of our time doing something with ourselves. In my case, physics, in your case, I don't know, whatever it is, machine learning and this. Yeah, you should have fun. What was... Wait, wait, wait. Follow your dreams. What dream did you have? Because there's... Well, originally, I was... Because you didn't follow your dream. I thought you were supposed to be a writer. I changed along the way. I was gonna be, but I changed. What happened? That was... What happened? Oh, I read... I decided to take the most serious literature course in my high school, which was a mistake. I'd probably be a second rate writer now. And... Could be a Nobel Prize winning writer. And the book that we read, even though I had read Russian novels, I was 15, I think, cured me from being a novelist. Destroyed your dream? Yes. Cured you. Okay. What was the book? Moby Dick. Okay. So, why Moby Dick? Yeah, why? So, I've read it since, and it's a great novel. Maybe it's as good as the Russian novels. I've never made it through. It was too boring. It was too long. Okay. Your words are gonna mesh with what I say. Excellent. And you may have the same problem at older ages. That's why I'm not a writer. It may be. So, the problem is, Moby Dick is... What I remember was there was a chapter that was maybe 100 pages long, all describing this, why there was Ahab and the white whale, and it was the battle between Ahab with his wooden peg leg and the white whale. And there was a chapter that was 100 pages long in my memory, I don't know how long it really was, that described in detail, though, great white whale and what he was doing and what his fins were like and this and that. And it was so incredibly boring, the word you used, that I thought, if this is great literature, screw it. Fascinating. Okay. And now, why did I have a problem? I know now in reflection, because I still read a lot, and I read that novel after I was 30 or 40 years old, and the problem was simple. I diagnosed what the problem was. That novel, in contrast to the Russian novels, which are very realistic and point of view, is one huge metaphor. At 15 years old, I probably didn't know the word, and I certainly didn't know the meaning of metaphor. Yeah, like, why do I care about a fish? Why are you telling me all about this fish? Exactly. It's one big metaphor. So, reading it later as a metaphor, I could really enjoy it. But the teacher gave me the wrong book, or maybe it was the right book because I went into physics. But it was truly, I think, I may oversimplify, but it was really that I was too young to read that book. Not too young to read the Russian novels, interestingly, but too young to read that because I probably didn't even know the word, and I certainly didn't understand it as a metaphor. Well, in terms of fish, I recommend people read Old Man and the Sea, much shorter, much better. It's still a metaphor, though. But you can read it just as a story about a guy catching a fish, and it's still fun to read. I had the same experience as you, not with Moby Dick, but later in college, I took a course on James Joyce. Don't ask me why. I was majoring in computer science, I took a course on James Joyce. And I was kept being told that he is widely considered, by many considered, to be the greatest literary writer of the 20th century. And I kept reading, I think, so his short story is The Dead, I think it's called. It was very good. Well, not very good, but pretty good. And then Ulysses. It's actually very good. It is very good. Only The Dead, the final story, it still rings with me today. But then Ulysses was, I got through Ulysses with the help of some Cliff Notes and so on. And so I did Ulysses and then Finnegan's Wake. The moment I started Finnegan's Wake, I said, this is stupid. That's when I went full into like, I don't know, that's when I went full Kafka, Bukowski, like people who just talk about the darkness of the human condition in the fewest words possible and without any of the music of language. So it was a turning point as well. I wonder when is the right time to appreciate the beauty of language. Like even Shakespeare. I was very much off put by Shakespeare in high school and only later I started to appreciate its value in the same way. Let me ask you a ridiculous question. Okay. I mean, because you've read Russian literature, let me ask this one last question. I might be lying. There might be a couple more, but what do you think is the meaning of this whole thing? You got a Nobel prize for looking out into the, trying to reach back into the beginning of the universe, listening to the gravitational waves, but that still doesn't answer the why. Why are we here? Beyond just the matter and anti matter, the philosophical question. The philosophical question about the meaning of life, I'm probably not really good at. I think that the individual meaning, I would say it rather simplistically is whether you've made a difference, a positive difference, I'd say for anything besides yourself. Meaning you could have been important to other people or you could have discovered gravitational waves that matters to other people or something, but something beyond just existing on the earth as an individual. So your life has meaning if you have affected either knowledge or people or something beyond yourself. It's a simplistic statement, but it's about as good as I can say. In all of its simplicity, it may be very true. Does it make you sad that this ride ends? Do you think about your mortality? Are you afraid of it? Not exactly afraid of it, but saddened by it. I'm old enough to know that I've lived most of my life and I enjoy being alive. I can imagine being sick and not wanting to be alive, but I'm not. It's been a good ride. I'm not happy to see it come to an end. I'd like to see it prolong, but I don't fear the dying itself or that kind of thing. It's more, I'd like to prolong what is I think a good life that I'm living and still living. It's sad to think that the finiteness of it is the thing that makes it special. And also sad to me, at least it's kind of, I don't think I'm using too strong of a word, but it's kind of terrifying the uncertainty of it. The mystery of it, the mystery of death. The mystery of it, yeah, of death. When we're talking about the mystery of black holes that's somehow distant, that's somehow out there and the mystery of our own. But even life, the mystery of consciousness, I find so hard to deal with too. I mean, it's not as painful. I mean, we're conscious, but the whole magic of life we can understand, but consciousness where we can actually think and so forth. It's pretty. It seems like such a beautiful gift that it really sucks that we get to let go of it. We have to let go of it. What do you hope your legacy is? As I'm sure they will. Aliens when they visit and humans have destroyed all of human civilization. Aliens read about you in an encyclopedia that we'll leave behind. What do you hope it says? Well, I would hope they, to the extent that they evaluated me, felt that I helped move science forward as a tangible contribution and that I served as a good role model for how humans should live their lives. And we're part of creating one of the most incredible things humans have ever created. So yes, there's the science. That's the Fermi thing, right? And the instrument, I guess. And the instrument. The instrument is a magical creation, not just by a human, by a collection of humans. The collaboration is, that's humanity at its best. I do hope we last quite a bit longer, but if we don't, this is a good thing to remember humans by. At least they built that thing. That's pretty impressive. Barry, this is an amazing conversation. Thank you so much for wasting your time and explaining so many things so well. I appreciate your time today. Thank you. Thanks for listening to this conversation with Barry Barish. To support this podcast, please check out our sponsors in the description. And now let me leave you with some words from Werner Heisenberg, a theoretical physicist and one of the key pioneers of quantum mechanics. Not only is the universe stranger than we think, it is stranger than we can think. Thank you for listening and hope to see you next time. let it out. And this is called general relativity. It's a new theory of gravity. 1915. In 1916, Einstein wrote a little paper where he did not do some fancy derivation. Instead, he did what I would call he used his intuition, which he was very good at too. And that is he noticed that if he wrote the formulas for general relativity in a particular way, they looked a lot like the formulas for electricity and magnetism. Being Einstein, he then took the leap that electricity and magnetism, we discovered only 20 years before that in the 1880s, have waves. Of course, that's light and electromagnetic waves, radio waves, everything else. So he said, if the formulas look similar, then gravity probably has waves too. That's such a big leap, by the way. I mean, maybe you could go back to the 1880s, maybe you can correct me, but that just seems like a heck of a leap. Yeah. And it was considered to be a heck of a leap. So first that paper was, except for this intuition, was poorly written, had a serious mistake. It had a factor of two wrong in the strength of gravity, which meant if we use those formulas, we would... And two years later, he wrote a second paper. And in that paper, it turns out to be important for us because in that paper, he not only fixed his factor of two mistake, which he never admitted, he just wrote it, fixed it like he always did. And then he told us how you make gravitational waves, what makes gravitational waves. And you might recall in electromagnetism, we make electromagnetic waves in a simple way. You take a plus charge and minus charge, you oscillate like this, and that makes the electromagnetic waves. And a physicist named Hertz made a receiver that could detect the waves and put it in the next room. He saw them and moved forward and backward and saw that it was wave like. So Einstein said, it won't be a dipole like that, it'll be a four pole thing. And that's what it's called, it's called a quadrupole moment that gives the gravitational wave. So that again, by insight, not by derivation. That set the table for what you needed to do to do it. At the same time, in the same year, Schwarzschild, not Einstein, said there were things called black holes. So it's interesting that that came the same. So what year was that? 1915. It was in parallel... Well, I should probably know this, but did Einstein not have an intuition that there should be such things as black holes? That came from Schwarzschild. Oh, interesting. Yeah. So Schwarzschild, who was a German theoretical physicist, he got killed in the war, I think, in the First World War, two years later or so. He's the one that proposed black holes, that there were black holes. That feels like a natural conclusion of general relativity, no? Or is that not? Well, it may seem like it, but I don't know about a natural conclusion. It's a result of curved space time though. Right. But it's such a weird result that you might have to... It's a special... Yeah, it's a special case. Yeah. So I don't know. Anyway, Einstein then, an interesting part of the story is that Einstein then left the problem. Most physicists, because it really wasn't derived, he just made this, didn't pick up on it or general relativity much because quantum mechanics became the thing in physics. And Einstein only picked up this problem again after he immigrated to the US. So he came to the US in 1932. And I think in 1934 or 1935, he was working with another physicist called Rosen, who he did several important works with, and they revisited the question. And they had a problem that most of us as students always had, that study general relativity. General relativity is really hard because it's four dimensional instead of three dimensional. And if you don't set it up right, you get infinities, which don't belong there. We call them coordinate singularities as a name. But if you get these infinities, you don't get the answers you want. And he was trying to derive now general relativity from general relativity, gravitational waves. And in doing it, he kept getting these infinities. And so he wrote a paper with Rosen that he submitted to our most important journal, Physical Review Letters. And that when it was submitted to Physical Review Letters, it was entitled, Do Gravitational Waves Exist? A very funny title to write 20 years after he proposed they exist. But it's because he had found these singularities, these infinities. And so the editor at that time, and the part of it that I don't know, is peer review. We live and die by peer review as scientists send our stuff out. We don't know when peer review actually started or what peer review Einstein ever experienced before this time. But the editor of Physical Review sent this out for review. He had a choice. He could take any article and just accept it. He could reject it, or he could send it for review. I believe the editors used to have much more power. Yeah, yeah. And he was a young man. His name was Tate. And he ended up being editor for years. So he sent this for review to a theoretical physicist named Robertson, who was also in this field of general relativity, who happened to be on sabbatical at that moment at Caltech. Otherwise, his institution was Princeton, where Einstein was. And he saw that the way they set up the problem, the infinities were like I make it as a student, because if you don't set it up right in general relativity, you get these infinities. And so he reviewed the article and gave an illustration that if they set it up in what are called cylindrical coordinates, these infinities went away. The editor of Physical Review was obviously intimidated by Einstein. He wrote this really not a letter back like I would get saying, you're screwed up in your paper instead. It was kind of, what do you think of the comments of our referee? Einstein wrote back, and it's a well documented letter, wrote back a letter to Physical Review saying, I didn't send you the paper to send it to one of your so called experts. I sent it to you to publish. I withdraw the paper. And he never published again in that journal. That was 1936. Instead, he rewrote it with the fixes that were made, changed the title and published it in what was called the Franklin Review, which is the Franklin Institute in Philadelphia, which is Benjamin Franklin Institute, which doesn't have a journal now, but did at that time. So the article is published. It's the last time he ever wrote about it. It remained controversial. So it wasn't until close to 1960, 1958, where there was a conference that brought together the experts in general relativity to try to sort out whether it was true that there were gravitational waves or not. And there was a very nice derivation by a British theorist from the heart of the theory that gets gravitational waves. And that was number one. The second thing that happened at that meeting is Richard Feynman was there. And Feynman said, well, if there's typical Feynman, if there's gravitational waves, they need to be able to do something, otherwise they don't exist. So they have to be able to transfer energy. So he made an idea of a gedankenexperiment that is just a bar with a couple of rings on it. And then if a gravitational wave goes through, it distorts the bar and that creates friction on these little rings and that's heat and that's energy. So that meant... Is that a good idea? That sounds like a good idea. Yeah. It means that he showed that that with the distortion of space time, you could transfer energy just by this little idea. And it was shown theoretically. So at that point, it was believed theoretically then by people that gravitational waves should exist. No, we should be able to detect them. We should be able to detect them, except that they're very, very small. And so what kind of, there's a bunch of questions here, but what kind of events would generate gravitational waves? You have to have this, what I call quadrupole moment. That comes about if I have, for example, two objects that go around each other like this, like the earth around the sun or the moon around the earth, or in our case, it turns out to be two black holes going around each other like this. So how's that different than basic oscillation back and forth? Is it just more common in nature to have... Oscillation is a dipole moment. So it has to be in three dimensional space kind of oscillation. So you have to have something that's three dimensional that'll give what I called a quadrupole moment. That's just built into this. And luckily in nature you have stuff... And luckily things exist. And it is luckily because the effect is so small that you could say, look, I could take a barbell and spin it, right? And detect the gravitational waves. But unfortunately, no matter how much I spin it, how fast I spin it, so I know how to make gravitational waves, but they're so weak, I can't detect them. So we have to take something that's stronger than I can make. Otherwise we would do what Hertz did for electromagnetic waves. Go in our lab, take a barbell, put it on something, spin it. Can I ask a dumb question? So a single object that's weirdly shaped, does that generate gravitational waves? So if it's rotating? Sure. But it's just a much weaker signal. It's weaker. Well, we didn't know what the strongest signal would be that we would see. We targeted seeing something called neutron stars actually, because black holes we don't know very much about. It turned out we were a little bit lucky. There was a stronger source, which was the black holes. Well, another ridiculous question. So you say waves. What does a wave mean? Like the most ridiculous version of that question is, what does it feel like to ride a wave as you get closer to the source? Or experience it? Well, if you experience a wave, imagine that this is what happens to you. I don't know what you mean about getting close. It comes to you. So it's like this light wave or something that comes through you. So when a light hits you, it makes your eyes detect it. I flashed it. What does this do? It's like going to the amusement park, and they have these mirrors. You look in this mirror and you look short and fat, and the one next to you makes you tall and thin. Imagine that you went back and forth between those two mirrors once a second. That would be a gravitational wave with a period of once a second. If you did it 60 times a second, go back and forth. And then that's all that happens. It makes you taller and shorter and fatter back and forth as it goes through you at the frequency of the gravitational wave. So the frequencies that we detect are higher than one a second, but that's the idea. And the amount is small. Amount is small, but if you're closer to the source of the wave, is it the same amount? Yeah, it doesn't dissipate. It doesn't dissipate. Okay, so it's not that fun of an amusement ride. Well, it does dissipate, but it's proportional to the distance. Right. It's not a big power. Right. Gotcha. But it would be a fun ride if you get a little bit closer or a lot closer. I mean, I wonder what the... Okay, this is a ridiculous question, but I have you here. I mean, the getting fatter and taller, I mean, that experience, for some reason, that's mind blowing to me because it brings the distortion of space time to you. I mean, space time is being morphed, right? Like this is a wave. That's right. That's so weird. And we're in space, so we're affected by it. Yeah, we're in space and now it's moving. It's moving. I don't know what to do with it. I mean, does it... Okay. How much do you think about the philosophical implications of general relativity? Like that we're in space time and it can be bent by gravity. Like, is that just what it is? Are we supposed to be okay with this? Because like Newton, even Newton is a little weird, right? But that at least like makes sense. That's our physical world. When an apple falls, it makes sense. But the fact that entirety of the space time we're in can bend, that's really mind blowing. Let me make another analogy. This is a therapy session for me at this point. Yeah, right. Another analogy. Thank you. So imagine you have a trampoline. Yes. Okay. What happens if you put a marble on a trampoline? It doesn't do anything, right? No. Just a little bit, but not much. Yeah. I mean, just if I drop it, it's not going to go anywhere. Now imagine I put a bowling ball at the center of the trampoline. Now I come up to the trampoline and I put a marble on, what happens? It'll roll towards the bowling ball. Okay. All right. So what's happened is the presence of this massive object distorted the space that the trampoline did. This is the same thing that happens to the presence of the earth, the earth and the apple. The presence of the earth affects the space around it, just like the bowling ball on the trampoline. Yeah. This doesn't make me feel better. I'm referring from the perspective of an ant walking around on that trampoline. Then some guy just dropped a ball and then not only dropped the ball, right? It's not just dropping a bowling ball. It's making the ball go up and down or doing some kind of oscillation thing where it's like waves. And that's so fundamentally different from the experience on being on flatland and walking around and just finding delicious, sweet things as ant does. And it just feels like to me from a human experience perspective, completely, it's humbling. It's truly humbling. It's humbling, but we see that kind of phenomenon all the time. Let me give you another example. Imagine that you walk up to a still pond. Yes. Okay. Now I throw, you throw a rock in it, what happens? The rock goes in, sinks to the bottom, fine. And these little ripples go out and they travel out. That's exactly what happens. I mean, there's a disturbance, which is these, say, the bowling ball or black holes. And then the ripples that go out in the water, they're not, they don't have any, they don't have the rock, any part, pieces of the rock. See, the thing is, I guess what's not disturbing about that is it's a, I mean, I guess a flat two dimensional surface that's being disturbed. Like for a three dimensional surface, a three dimensional space to be disturbed feels weird. It's even worse. It's four dimensional because it's space and time. Time, yeah. So that's why you need Einstein is to make it four dimensional. To make it okay? No, to make it. To make it four dimensional? Yeah. Yeah, to take the same phenomenon and look at it in all of space and time. Anyway, luckily for you and I and all of us, the amount of distortion is incredibly small. So it turns out that if you think of space itself, now this is going to blow your mind too, if you think of space as being like a material, like this table, it's very stiff. You know, we have materials that are very pliable, materials that are very stiff. So space itself is very stiff. So when gravitational waves come through it, luckily for us, it doesn't distort it so much that it affects our ordinary life very much. No, I mean, that's great. That's great. I thought there was something bad coming. No, this is great. That's great news. So I mean, that, I mean, perhaps we evolved as life on Earth to be such that for us, this particular set of effects of gravitational waves is not that significant. Maybe that's why. It is. You probably used this effect today or yesterday. Did what? So it's pervasive. Well, because... You mean gravity or the way, or external? Because I only... Curvature of space and time. Curvature of space. How? I only care, a person is a human, right? The gravity of Earth. But you use it every day, almost. Oh, it's curving. Uh huh. No, no, no. No, no, no. It's in this thing. Every time it tells you where you are, how does it tell you where you are? It tells you where you are because we have 24 satellites or some number that are going around in space and it asks how long it takes the beam to go to the satellite and come back, the signal, to different ones. And then it triangulates and tells you where you are. And then if you go down the road, it tells you where you are. Do you know that if you did that with the satellites and you didn't use Einstein's equations? Oh no. You won't get the right answer. That's right. And in fact, if you take a road that's, say, 10 meters wide, I've done these numbers, and you ask how long you'd stay on the road if you didn't make the correction for general relativity, this thing you're poo pooing, because you're using every day, you'd go off the road in about a minute. Well, actually, that might be my problem. So you use it. So don't poo poo it. Well, I think I'm using an Android, so maybe, and the GPS doesn't work that well, so maybe I'm using Newton's physics. So I need to upgrade to general relativity. So gravitational waves and Einstein had, wait, Feynman really does have a part in the story? Yeah. Was that one of the first kind of experimental proposed to detect gravitational waves? Well, he did what we call a Godonkin experiment. That's a thought experiment. Yes. Okay. Not a real experiment. But then after that, then people believe gravitational waves must exist. You can kind of calculate how big they are. They're tiny. And so people started searching. The first idea that was used was Feynman's idea, and the very end of it. And it was to take a great big, huge bar of aluminum and then put around, and it's made like a cylinder, and then put around it some very, very sensitive detectors so that if a gravitational wave happened to go through it, it would go, and you'd detect this extra strain that was there. And that was this method that was used until we came along. It wasn't a very good method to use. And what was the, so we're talking about a pretty weak signal here. Yeah, that's why that method didn't work. So what, can you tell the story of figuring out what kind of method would be able to detect this very weak signal of gravitational waves? So remembering what happens when you go to the amusement park, that it's going to do something like stretch this way and squash that way, squash this way and stretch this way. We do have an instrument that can detect that kind of thing. It's called an interferometer. And what it does is it just basically takes, usually light, and the two directions that we're talking about, you send light down one direction and the perpendicular direction. And if nothing changes, it takes the same, and the arms are the same length, it just goes down, bounces back. And if you invert one compared to the other, they cancel so that nothing happens. But if it's like the amusement park and one of the arms got shorter and fatter, so it took longer to go horizontally than it did to go vertically, then when the light comes back, that comes back somewhat out of time. And that basically is the scheme. The only problem is that that's not done very accurately in general, and we had to do it extremely accurately. So what's the difficulty of doing so accurately? Okay. So the measurement that we have to do is a distortion in time. How big is it? It's a distortion that's one part in 10 to the 21. That's 21 zeros and a one. Okay. So this is like a delay in the thing coming back? One of them coming back after the other one, but the difference is just one part in 10 to the 21. So for that reason, we make it big, let the arms be long. Okay, so one part in 10 to the 21. In our case, it's kilometers long. So we have an instrument that's kilometers in one direction, kilometers in the other. How many kilometers are we talking about? Four kilometers. Four kilometers in each direction. If you take then one part in 10 to the 21, we're talking about measuring something to 10 to the minus 18 meters. Okay. Now, to tell you how small that is, the proton thing we're made of, which you can't go and grab so easily, is 10 to the minus 15 meters. So this is one one thousandth the size of a proton. That's the size of the effect. Einstein himself didn't think this could be measured. We've never seen, actually, he said that. But that's because he didn't anticipate modern lasers and techniques that we developed. Okay. So maybe can you tell me a little bit what you're referring to as LIGO, the Laser Interferometer Gravitational Wave Observatory. What is LIGO? Can you just elaborate kind of the big picture view here before I ask you specific questions about it? Yeah. So in the same idea that I just said, we have two long vacuum pipes, four kilometers long. We start with a laser beam and we divide the beam going down the two arms. And we have a mirror at the other end, reflects it back. It's more subtle, but we bring it back. If there's no distortion in space time and the lengths are exactly the same, which we calibrate them to be, then when it comes back, if we just invert one signal compared to the other, they'll just cancel. So we see nothing. Okay. But if one arm got a little bit longer than the other, then they don't come back at exactly the same time. They don't exactly cancel. That's what we measure. So to give a number to it, we have the change of length to be able to do this 10 to the minus 18 meters to one part in 10 to the 12th. And that was the big experimental challenge that required a lot of innovation to be able to do. You gave a lot of credit to, I think, Caltech and MIT for some of the technical developments within this project. Is there some interesting things you can speak to at the low level of some cool stuff that had to be solved? I'm a software engineer, so I have so much more respect for everything done here than anything I've ever done. So I'll give you an example of doing mechanical engineering at a better, basically mechanical engineering and geology and maybe at a level. So what's the problem? The problem is the following, that I've given you this picture of an instrument that by some magic, I can make good enough to measure this very short distance. But then I put it down here, it won't work. And the reason it doesn't work is that the Earth itself is moving all over the place all the time. You don't realize it, it seems pretty good to you, but it's moving all the time. So somehow it's moving so much that we can't deal with it. We happen to be trying to do the experiment here on Earth, but we can't deal with it. So we have to make the instrument isolated from the Earth at the frequencies we're at. We've got to float it. That's an engineering problem, not a physics problem. So we're having a conversation on a podcast right now, and people who record music work with this, how to create an isolated room. And they usually build a room within a room, but that's still not isolated. In fact, they say it's impossible to truly isolate from sound, from noise and stuff like that. But that's like one step of millions that you took is building a room inside a room, because you basically have to isolate all. No, this is actually an easier problem. You just have to do it really well. So making a clean room is really a tough problem because you have to put a room inside a room. This is really simple engineering or physics. Okay, so what do you have to do? How do you isolate yourself from the Earth? First, we work at, we're not looking at all frequencies for gravitational waves. We're looking at particular frequencies that you can deal with here on Earth. So what are frequencies would those be? You were just talking about frequencies. We know by evolution, our bodies know, it's the audio band. Okay, the reason our ears work where they work is that's where the Earth isn't going, making too much noise. Okay, so the reason our ears work the way they work is because this is where it's quiet. That's right. So if you go to one Hertz instead of 10 Hertz, the Earth is really moving around. So somehow we live in what we call the audio band. It's tens of Hertz to thousands of Hertz. That's where we live, okay? If we're going to do an experiment on the Earth, it's the same frequency. That's where the Earth is the quietest. So we have to work in that frequency. So we're not looking at all frequencies, okay? So the solution for the shaking of the Earth to get rid of it is pretty mundane if we do the same thing that you do to make your car drive smoothly down the road. So what happens when your car goes over a bump? Early cars did that, they bounced. Right. Okay, but you don't feel that in your car. So what happened to that energy? You can't just disappear energy. So we have these things called shock absorbers in the car. What they do is they take the thing that went like that, and they basically can't get rid of the energy, but they move it to very, very low frequency. So what you feel isn't, you feel it go smoothly, okay? All

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