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肖恩·卡羅爾:量子力學與多世界詮釋

Sean Carroll: Quantum Mechanics and the Many-Worlds Interpretation

物理學家解釋多世界詮釋為何更簡潔,以及它如何重塑我們對機率與現實的看法。

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牛頓發明了經典力學。你扔一塊石頭,他能算出石頭會飛到哪裡。三百年後,我們還在用他這套理論把探測器送上火星。

牛頓自己知道,他的理論裡藏著一個解釋不了的東西:地球怎麼知道九千三百萬英里外有個太陽在拉它?

他給出的回答堪稱物理學史上最誠實的甩鍋:這個問題,我留給後人去想,因為我不知道答案。

牛頓沒說出口的那個漏洞

超距作用(action at a distance)讓牛頓很不舒服。太陽遠在天邊,沒有繩子,沒有彈簧,憑什麼隔空對地球施加引力?這在人的直覺層面說不通。

肖恩·卡羅爾(Sean Carroll)在這期訪談裡講了一段很少被提及的細節。牛頓不只是擔心超距作用,他還幾乎發明了混沌理論。當他用萬有引力解釋行星運動時,只要算地球繞太陽就夠了。可他知道,一旦把木星和土星的引力也算進去,整個太陽系的軌道會亂掉。

牛頓的解決辦法是:上帝會時不時出手,把跑偏的行星撥回正軌。這樣太陽系才能穩定存在下去。

這聽起來像宗教補丁,但它反映了一個真實的困境。當你手裡只有一套理論,而這套理論在某些地方明顯不夠用時,人會本能地找一個外部力量來填坑。牛頓用的是上帝,今天我們用的是別的詞。

後人怎麼把漏洞補上

大約1800年,拉普拉斯給出了答案。他把牛頓的引力改寫成場論。太陽不再隔空拽地球,兩者之間瀰漫著一個引力場,這個場按照一個方程(拉普拉斯方程)演化,一步步把影響傳遞過去。

奇妙的地方在於,同一套理論換一種數學語言,做出完全相同的預言。超距作用在牛頓引力裡本來就不是必需品,你可以用場來表述它。

愛因斯坦往前走了一步。廣義相對論裡當然也有場,但多了一樣東西:光速。場的變化不能瞬間傳遍宇宙。你在這裡晃一下,引力擾動以光速向外輻射,這就是引力波。2015年LIGO真的探測到了。

如果最後發現物理學裡確實存在超距作用,而這是描述世界最好的方式,那我就按這個方式來。(肖恩·卡羅爾)

卡羅爾這句話可以停下來想一想。他是在說,不要因為直覺上不喜歡某個答案就否定它。牛頓不喜歡超距作用,但他沒有因此拒絕自己的理論。這個態度在量子力學裡會變得極其重要,因為那裡有更多讓人本能抗拒的結論。

人類的理解有沒有天花板

喬姆斯基有個觀點:人的認知能力是進化出來的,受生物學約束,所以存在硬性上限。

卡羅爾不完全同意這個悲觀版本。他區分了兩件事。

第一,我們有能力做形式化的符號操作。人類跨過了這道門檻,狗和貓沒有。一旦你能在腦子裡裝下一套邏輯結構並操作它,理解就不再依賴“能不能在腦中畫出來”。

愛德華·威滕證明的定理涉及上百維的數學空間。他當然沒法在腦子裡看見那個空間。他做的是數學。但這不妨礙他理解結果。

第二,計算能力有極限,理解能力未必有。沒人能心算百萬位數的立方根,這是計算限制,不是理解限制。

卡羅爾舉了個反問:500年前去問當時最聰明的人“我們是否接近理解自然的極限”,他們會怎麼回答?他們連經典力學都還沒有,更別說量子力學。

“在所有讓我睡不著覺的擔憂裡,人類理性無法理解世界這一條排名很靠後。”

物理學裡最美的想法

卡羅爾選了動量守恆。

亞里士多德在《物理學》裡寫下一個日常觀察:推一下瓶子,瓶子動;鬆手,瓶子停。這件事在你家客廳裡重複無數次,看起來無可辯駁。

亞里士多德由此構建了一整套世界觀:萬物有各自的本性(nature),有它們想去的地方(目的論,teleology)。你推瓶子,是把它推離了它本該待的位置,所以它要停下來。

這套解釋撐了一千五百年。直到有人提出:如果沒有摩擦、沒有空氣阻力、沒有耗散,物體的自然狀態是以恆定速度一直直線運動下去。

動量守恆。就這麼簡單。

卡羅爾說,這個想法之所以深刻,跟它對不對是兩碼事。它換掉了整個提問方式。

在亞里士多德的框架裡,你必須問“為什麼”。這個東西為什麼這樣動?它的本性是什麼?它的目的是什麼?

有了動量守恆,你不需要問為什麼。你給我今天世界的狀態,我能算出它明天在哪、昨天在哪。它是非人格的,沒有目標,不指向任何未來。它只是在按照模式運轉。

“這比經典力學或者量子力學本身更深刻,是現代科學得以起步的那個洞見。你不需要本性,不需要目的,你只需要一些模式。”

這個轉變花了很久。公元1000年左右,波斯黃金時代的伊本·西那(Ibn Sina)已經接近了這個想法。他設想真空中拋射物會勻速運動。可他並不喜歡這個結論,用法跟薛定諤後來用那隻貓一樣:你們不會真信這個吧?因為如果真有真空,東西就會永遠動下去。

從伊本·西拿到牛頓,又過了六百年。

數學和物理到底是什麼關係

卡羅爾給了一個很乾淨的定義:數學研究所有可能世界的邏輯結構,物理研究我們所在的這一個。

維格納(Eugene Wigner)問過“數學在物理中為何如此有效”。卡羅爾覺得這個問題問偏了。任何可能的世界,你都能用數學描述。真正讓人吃驚的地方在別處:數學簡單到能寫在一件T恤上。

巨大的資訊壓縮,而且壓縮後的結果在真實世界裡成立。

“我們這個世界有個奇怪的事實。你可以希望去解釋它,也可以把它當作一個赤裸裸的事實接受下來。”

他傾向於後者。世界存在這件事本身,以及具體的物理定律為什麼是這套而不是別的,可能沒有更深層的解釋。到了某個層面,你只能說:就是這樣。

什麼是基本的,什麼是湧現的

卡羅爾用一張桌子講清楚了這個問題。

你可以用桌子的語言描述它:高度、寬度、材質、重量、結實程度。這非常有用。

你也可以用原子的語言描述它:一大堆原子按某種方式排列。

區別在哪?把桌子砸碎。你還能用原子的語言描述這堆碎片,但你沒法再叫它桌子了。

“理論越基本,它的有效範圍就越廣。原子的語言比桌子的語言更全面。”

判斷哪個更基本,有個可操作的判據:把它拆掉,看哪個描述還能活下來。越基本的東西,能活下來的場景越多。

現在我們知道的層級大致是:細胞、器官比原子分子更湧現;原子分子比量子場更湧現。會不會有底?不知道。卡羅爾猜有,世界總得有個不能再往下問的地方。

回到最開始:量子力學是什麼

經典力學裡,物體有位置、有速度。你知道所有東西的位置和速度,就能算出一切。

量子力學表面上很像。有一個東西叫量子態或者波函式,有一個方程支配它怎麼變。那個方程是薛定諤方程,不是牛頓定律。波函式是個波,嚴格說是高維向量空間裡的一個向量。

麻煩出在第二套規則上。教科書版本的量子力學在薛定諤方程之外,還加了一堆關於“觀察”“測量”的規則。

經典力學裡沒有觀察規則。你看一眼,看到什麼就是什麼,不會改變系統。

量子力學裡,測量被賦予了一種根本性的地位。電子在原子裡的波函式是散開的雲,但你看它的時候,你看到的是一個有確定位置的點。測量瞬間改變了它的狀態,而且這個改變會影響它之後的行為。

“這裡要小心,因為我們並不一致同意量子力學到底在說什麼。所以我說的是教科書版本。”

原子、電子,還有那個愚蠢的名字

原子的概念是化學家先搞出來的。1800年代,他們發現氧化錫有兩種,其中一種的氧含量正好是另一種的兩倍。為什麼是兩倍,不是1.5倍?

道爾頓說:因為一種是一個錫原子配一個氧原子,另一種是一個錫原子配兩個氧原子。

這是猜測,是假說。但基於這個假說,你能做出新預言。化學家很快相信原子是真的。物理學家慢得多。玻爾茲曼一生都在為原子辯護,因為他在德國工作,那裡不流行原子論。

盧瑟福後來發現原子還能再分。原子中心是原子核,由質子和中子組成,質量差不多是電子的八百倍。電子很輕,但原子的化學性質、電、光,幾乎全靠電子在工作。

然後問題來了。如果電子像小行星一樣繞著原子核轉圈,它就會輻射電磁波。你可以算它多久會螺旋墜入原子核:10的負11次方秒。一千億分之一秒。

“所以這個影象肯定不對。”

另一邊,人們已經知道光(公認的波)有粒子性質。那反過來,公認的粒子(電子)會不會有波的性質?

於是有人提出:別把電子想成繞圈的小點,把它想成彌散的波。他們給這個東西起名叫波函式。

卡羅爾的評價:宇宙中最深刻的東西之一,得了個世界上最蠢的名字。

波函式的意思是:空間每一點上有一個數,代表電子在那裡的波函式值。

而且只有一個波函式。兩個電子各自有一個波函式,這種說法是錯的,它們共享一個聯合波函式。再往外推,整個宇宙只有一個波函式。

糾纏:量子力學裡最不像經典的地方

按教科書說法,波函式平方一下,得到的是在那個位置觀察到系統的機率。

兩個電子共享一個波函式,這個波函式告訴你同時觀察兩個電子會得到什麼的機率。

可以設計出這樣一種狀態:你不知道任何一個電子會在哪被看到,但你知道它們一定會在同一個地方被看到。

這就是糾纏。它裡面有一個條件句:如果我在某個位置看到其中一個,我就知道另一個在做什麼。

經典力學裡沒有這種事。兩個粒子就是分開的,你對一個的無知和對另一個的無知是獨立的兩件事。

有個常見的誤解,以為糾纏和距離有關。並沒有。兩個電子可以完全糾纏,也可以完全不糾纏,跟它們相距多遠沒有關係。

但在量子場論的影象裡,空間本身充滿了振動的場。兩個靠得很近的場會高度糾纏,離得遠就不糾纏。這是場與場之間的糾纏,跟單對粒子的糾纏是兩回事。

“空無一物的空間”其實不空。就在你現在坐的位置,有一個引力場,你扔個東西就能探測到它。你看不見它,但它在。

希爾伯特空間和熵,用日常語言說清楚

希爾伯特空間是所有可能波函式的空間。它是一個抽象空間,跟我們在裡面生活的三維空間沒有直接關係。

維度是什麼意思?就是你需要給我多少個數字,才能完整指定系統的狀態。

經典力學裡,位置是三個數。加上速度,又是三個數。這叫相空間,六維。如果還有朝向,再加三個。

資訊越多,抽象空間的維度越高。

熵是什麼?一個粗略但好用的說法:它衡量我們對系統狀態有多少不知道。

一瓶水,你知道總體積、溫度、壓強。但你絕對不知道每個水分子確切的位置和速度。這部分未知資訊,就是熵在刻畫的東西。

希爾伯特空間越大,系統可能擁有的熵上限越高。

無窮,只有三個簡單的數

卡羅爾說了一句很有意思的話:簡單的數只有三個。零、一、無窮。

三百一十八這個數很古怪,你需要很多位元才能說清它是多少。但零、一、無窮,一旦你有了三百個東西,你其實和有無窮個東西差不多,除非你能說出在哪停下來。

“所以從某種意義上說,無窮是一個非常自然的、東西存在的數量。”

很多人把無窮當成數學家的方便工具,一種為了讓公式收斂而臨時塞進去的東西。卡羅爾的意思是反過來的:只要你不給東西設上限,無窮就是預設結果。

你寫五行程式碼,問它跑多久會停。答案是永遠。你沒打算引入無窮,無窮自己找上門來。

測量問題:教科書留了個洞

教科書量子力學把世界分成兩半:被觀察的系統,和觀察者。系統按薛定諤方程演化,但一測量,波函式坍縮,你看到一個確定結果。

這個“坍縮”是什麼?教科書沒說。它只是把測量當作一個不加解釋的原始概念塞進公理,然後所有的計算都圍著它轉。

卡羅爾的態度很明確:測量和觀察者不會在最終物理定律裡扮演基本角色。理由很樸素,到目前為止所有證據都指向這個方向。

“如果觀測真的在實在的本質裡扮演基本角色,那會酷到爆炸。但我沒看到任何證據。”

那怎麼辦?換一個不需要測量假設的解釋。

埃弗雷特只說兩件事

1950年代,普林斯頓的研究生休·埃弗雷特三世(Hugh Everett III)提出一個極簡方案。

第一,你,觀察者,也是一個量子系統。你沒什麼特別的。你是一堆原子,你有波函式,你服從薛定諤方程,跟別的東西一樣。

第二,當你以為自己在測量時,實際發生的是你與那個東西發生了糾纏。

電子波函式散在多個位置。你看它,只看到一個位置。真實發生的過程是這樣的:電子仍然在所有位置,但它現在與你的波函式糾纏在一起。波函式的一部分說“電子在這裡,你認為你在這看到了它”,另一部分說“電子在那裡,你認為你在那看到了它”。

這些不同的部分一旦產生,就不再互相交流、不再互相影響。它們像是彼此分離的世界。

“埃弗雷特做的與其說是物理,不如說是心理治療。他說:沒事的,你不需要那些額外規則,你只需要相信薛定諤方程。代價是外面有一大堆額外的世界。”

整個理論就這麼多。剩下的所有工作,都是如何把這個數學對映到我們觀察到的現實上。

怎麼切分世界?怎麼區分系統和環境?環境就是你沒在追蹤的所有自由度。你測一瓶水,追蹤體積和溫度,不追蹤每個分子、每個光子、房間裡每個空氣分子。那些就是環境。

世界什麼時候分裂?當一個處於疊加態的量子系統與環境發生糾纏的時候。不需要有觀察者在場。

分裂,不是複製

很多人擔心能量守恆:憑空多出一個世界,能量從哪來?

卡羅爾說這個問題有確定答案,而且毫無爭議:能量守恆,多世界不違反它。

問題出在“複製”這個詞上。用“分裂”更準確。

畫一個X軸和Y軸,畫一個長度為一、角度45度的向量。你可以把它寫成兩個向量的和,一個沿X,一個沿Y,每個長度是根號二分之一。

一個箭頭寫成兩個箭頭,總長度沒變。這只是換了一種描述方式。

宇宙的波函式是一個大向量。分裂的時候,向量被拆成幾部分,總量守恆。宇宙被拆分成了兩份更瘦的,總量沒變。憑空多出一份的那種影象,在數學上找不到依據。

“在其他問題上我承認有合理的疑問,比如機率到底從哪來。但能量守恆這個問題,我們知道答案。”

為什麼多世界讓人不舒服

卡羅爾區分了兩種簡單性。

理論本身的簡單性:這個理論按自己的規則描述世界有多簡潔。多世界在這裡贏了,它只有波函式和薛定諤方程。

對映的簡單性:把這個數學形式對應到我們看到的世界上有多容易。牛頓力學在這項上得分很高,瓶子就在那,質心就在那。廣義相對論難一點,時空曲率不太好想象。量子力學很難。多世界最難。

“所有研究多世界的工作,都花在如何把它對映到我們觀察到的世界上。所以對它感到不爽是完全正當的。但如果沒有替代方案,而這個理論一直管用,你最終應該克服這種不爽。”

問題是,現在有替代方案。

辯論臺上的三個領跑者

把量子力學解釋放到辯論臺上,會有十幾個候選人,但只有三個領跑者。

第一個是埃弗雷特的多世界。只有波函式,永遠服從薛定諤方程。

第二個是隱變數理論。波函式是真的,可它不構成實在的全部。還有別的東西,最簡單的版本里是粒子。量子系統看起來既像波又像粒子:多世界說它真的是波、在某些觀測條件下看起來像粒子;隱變數說它真的是既有波又有粒子,粒子被波函式推著走。麻煩在於,加上量子場論和量子引力之後,這套理論變得極其難搞。

第三個是自發坍縮理論。每個粒子每秒鐘都有一個小機率,波函式自發坍縮。對單個粒子來說這個機率小到幾億年才發生一次。但一張桌子裡有遠遠超過一億個粒子,而且它們互相糾纏。一個坍縮,會把周圍全帶下去。彭羅斯還有一個變種:當波函式兩部分的引力差異大到一定程度,波函式自動坍縮。

還有第四個類別,認識論解釋(epistemic interpretations)。它說波函式根本不是對實在的描述,只是預測實驗結果的工具。兩個人對同一個系統可以有不同的波函式,因為他們知道的東西不同。

麻煩在於:那它在預測什麼?如果波函式不描述任何實在的東西,預測的物件是什麼?認識論解釋在這裡選擇不回答。

卡羅爾為什麼站在多世界這邊

兩個理由。

第一,它最簡單。最赤裸、最精簡、最純粹的量子力學。卡羅爾願意在“把形式對映到現實”上花大力氣,不願意把形式本身搞複雜。

第二,也是更實用的理由:其他所有版本都帶著經典力學的包袱。

隱變數理論需要預設粒子在空間裡的位置。自發坍縮理論需要預設某種經典時空背景。當你研究量子引力、時空湧現、全息術的時候,這些預設會變成障礙。

“多世界是即插即用的。你給我一個理論,我就能給你它的多世界版本。其他解釋每換一個系統,你都得從頭搭一遍。”

所以在時空的經典描述明顯失效的地方,應該從最量子的那個理論出發,往上搭時空的模型。

時空可能只是近似

愛因斯坦1915到1916年把廣義相對論寫成最終形式。引力是時空的彎曲,有一個場遍佈宇宙,告訴我們時空彎了多少。這個場完全是經典的。

我們有一個演算法,可以把經典理論量子化。量子電動力學就是這麼來的。但這個過程會遇到無窮大,費曼、施溫格、朝永振一郎拿了諾貝爾獎教我們怎麼處理,威爾遜又拿了一個獎說這些無窮大本來就不該讓你擔心。

於是大家以為,量子引力也可以這麼搞:從經典廣義相對論出發,量子化它。

但引力的無窮大比電磁學的頑固得多,至今沒能成功。而且有證據表明,量子引力根本不是場論。它帶著某種我們還不理解的非局域特徵。這個線索來自黑洞、霍金輻射和資訊守恆。

如果基本理論連局域性都不是,那你根本不知道該從哪個經典前身出發去量子化。

“唯一合乎邏輯的做法是反過來:從內稟量子的東西開始,看能不能找到經典極限。”

黑洞把局域性逼到牆角

局域性是牛頓那個老問題的答案。場在這裡的值,只直接取決於緊挨著它的那些點的值。那些點又取決於它們的鄰居。影響可以跨越空間,但每一步都是區域性的。

這個原則寫進了每一個場論,包括廣義相對論。

黑洞讓它出了問題。霍金告訴我們黑洞會輻射,最終蒸發掉。如果你用某種東西造一個黑洞,然後讓整個系統按薛定諤方程演化,理論上你能預言它最後變成什麼。已經有很好的論證表明,這件事沒法在保持局域性的同時完成。資訊似乎以非局域的方式散佈出去了。

全息原理說的就是這個。從外部觀察者的角度看,落入黑洞的所有資訊被抹在視界上,一個二維表面編碼了整個三維內部。

還有一個配套的概念叫互補性。沒有唯一正確的方式描述黑洞內部發生了什麼。不同觀察者會給出不同描述,都準確,但聽起來互相矛盾。這個詞是從玻爾那裡借來的:你可以測位置,也可以測動量,不能同時測。

我感到解放。空間只是一個很好的近似。一旦你開始量子化引力,這件事遲早會成立。(肖恩·卡羅爾)

時間之箭是湧現的,時間不是

這裡要分清兩個東西。

時間和時間的箭頭,是兩件事。空間沒有箭頭,你不會覺得空間必須有個方向。時間可以有箭頭,也可以沒有。

如果宇宙處在一個熱平衡態,沒有時間箭頭,但時間仍然存在,此刻和未來仍然有區別。

時間箭頭是過去和未來的差別。它來自初始條件。

基本定律完全可逆。給我某一刻宇宙的狀態,我既能往前算也能往後算。定律裡沒有箭頭。

但140億年前大爆炸附近的初始條件很特殊:熵極低。從那以後熵一直在增加,宇宙變得更無序、更混亂。這是熱力學箭頭。

在量子力學裡,特殊初始條件表現為:波函式最初只有一個分支,然後宇宙一直在分支,分支越來越多。

“這是同一種箭頭。物理定律可逆,特殊初始條件製造了方向。”

卡羅爾說時間之箭是湧現的,時間本身他沒這麼說。這兩者常被混為一談。

這些理論怎麼檢驗

多世界的檢驗方式很間接。如果有實驗發現波函式會自發坍縮,那麼多世界就被排除了。這類實驗正在進行。

隱變數理論呢?有一個定理似乎表明它的預言永遠和多世界一樣。卡羅爾對這個定理有點懷疑,他說自己還沒把它內化成直覺的一部分,可能還有漏洞。

除此之外,就只剩“量子力學一路到底”。科學記者喜歡寫那種標題驚悚的文章:“量子力學被證明比我們想的更神奇”。其實還是1926年那套量子力學。

時空湧現那邊完全不同。理論還在極原始的階段,甚至還沒有一個能寫下來、像樣的、誠實的理論。所以完全可能存在我們還沒想到的實驗預言。

需要極大尺度,或者極快,或者極高能量。不知道。

有一種可能:不同波長的光速度不同。這跟超光速無關,是光速本身隨波長變化。如果真的存在,那是對現有物理的劇烈違反。但它不是理論的必然預言,問題就在這裡,理論還不夠成熟,說不出確定的話。

量子力學和意識基本沒關係

“量子”這個詞被濫用到除了量子力學以外的所有地方。卡羅爾對此很直接。

心智是相當經典的東西。不敢百分百確定,但不認為糾纏這類現象對人類心智或意識是關鍵的。

他是徹底的物理主義者。沒有獨立的心智狀態或心智屬性,它們都是湧現的,就像時空一樣。時空已經夠難理解了,意識還沒被理解,這絲毫不讓人意外。

有人會問,如果觀測在物理裡是基本的,那意識會不會也是基本的?卡羅爾的回答是:完全可能,但我不為此花時間。他的判斷依據始終是同一條,到目前為止證據都指向另一個方向。

做播客這件事

卡羅爾的播客叫 Mindscape。Lex 說這是他最喜歡的科學播客之一,因為卡羅爾不止講物理,還會跑到自己專業之外去問真正的問題。

卡羅爾承認,做播客的初衷有點自私:家裡堆了一摞沒讀的書,找不到時間讀。採訪作者能逼自己讀。

“這個方法完全有效。現在我有點煩人們寫那麼長的書。”

他說自己在學習怎麼當一個好採訪者。問題問得好,但一來一回的節奏還在練。有的對話他幾乎不說話,有的他說了一半時間,中間有個最佳點。

他學到最多的,恰恰是那些跟物理、哲學無關的話題。和溫頓·馬薩利斯聊爵士,和侍酒大師聊葡萄酒,和威爾·威爾金森聊黨派極化與城鄉分裂,和心理學家聊認知失調。

還有一次和斯科特·德里克森(《奇異博士》導演)聊了一整集大片製作流程。德里克森是福音派基督徒,他們也聊了實在的本質。卡羅爾說,他還想再請幾位真正懂神學的有神論者來聊,只是還沒安排上。

他零興趣請那種專門來被羞辱的靶子。不請地平說的人來“打臉”,不請江湖騙子。

“我願意請我不同意的人,但只請那些我認為聽眾能從中學到東西的人。”

Lex 問他,有沒有一些對話他希望卡羅爾多反駁幾句,聽眾會更爽。卡羅爾說這取決於嘉賓。和大衛·查爾默斯(David Chalmers)分歧很大,他會說清楚自己為什麼不同意,但不會糾纏,因為“我每週都有一集,你只上一次”。和菲利普·戈夫(Philip Goff)那集就真的槓上了,因為對方想槓。

這裡有個分寸問題。爭論好看,前提是雙方對彼此有基本的智力尊重。卡羅爾說他只想讓雙方都把話講清楚,不想為了節目效果製造衝突。

Lex 還拋了一個更難的判斷題:如果有人接受進化論的基本框架,但認為寒武紀大爆發這類現象現有理論解釋不了,那他是跳出框架的思考者,還是披著科學外衣的怪人?

卡羅爾坦言這問題他沒有滿意答案。離自己專業越遠,判斷越難。他說自己得去問那些他尊重、又真的懂行的人。而且他提醒了一句:物理學家有時對異見過於輕蔑,生物學家也一樣。

這本關於量子力學的書

新書叫《Something Deeply Hidden》。Lex 在開頭說,聽卡羅爾講糾纏、互補性、時空湧現,讓他想起鮑勃·羅斯(Bob Ross)教人畫畫的老電視節目。

卡羅爾是理論物理界的鮑勃·羅斯。這個比喻挺準,因為他的核心能力就是把極其抽象的東西講到你能在腦子裡搭出一個粗糙但有用的模型,然後告訴你哪裡粗糙、為什麼粗糙、哪些地方我們其實還不知道。

他沒有假裝量子力學已經被完全理解。他反覆說“我們不知道”“這不是板上釘釘”“我可能是錯的”。這種誠實比任何自信的斷言都更有說服力。

訪談裡他提到一個細節:如果有人問牛頓怎麼看這本書,可能要花幾個月補課。但也可能牛頓有心理障礙,根本沒法用這種方式看世界。畢竟他寫聖經和鍊金術的篇幅遠多於物理。

而伽利略,雖然比牛頓早,反而是更現代的思想者。把他帶到今天,六個月就能跟上進度,然後跑到你辦公室說你最新那篇論文哪裡錯了。

可以帶走的東西

這期對話資訊密度很高,散場之後能真正用上的,大概是下面這幾條。

  • 遇到一個反直覺但極其成功的理論,先別用直覺去否它。牛頓不喜歡超距作用,但沒因此扔掉自己的方程。後人花了兩百年發現,超距作用本來就不是必需品。直覺該更新的時候要更新,但在那之前別讓它擋住路。
  • 區分“理論本身簡單”和“理論對映到現實簡單”。多世界在第一條上贏了,第二條上輸了。你做技術選型時也會碰到同一種取捨:架構優雅但落地痛苦,還是架構笨重但心智負擔小。搞清楚自己在最佳化哪一項。
  • 判斷一個描述是基本還是湧現,有個可操作的檢驗:把它拆掉,看這個描述還成不成立。桌子砸碎了就不是桌子,原子還是原子。越基本的東西,能活下來的場景越多。
  • 別把“測量”當成理所當然的原始概念。任何理論裡出現一個不加解釋的黑箱,都值得追問它背後是什麼。教科書量子力學把測量放進公理,埃弗雷特把它拆掉了,換來一個更簡潔但更反直覺的世界圖景。
  • 無窮是你不設上限時的預設結果。問“這個系統會跑多久”,答案可能就是永遠。接受這一點,比硬給它安一個上限更接近真相。
  • 時間箭頭和時間的區別值得記住。定律可逆,方向來自初始條件。你在生活裡看到的所有“不可逆”,多半也來自某個特殊的起點,定律本身沒有在推你。
  • 如果要做內容,卡羅爾那條經驗可以直接抄:請那些你不同意但有真本事的人,只請那些聽眾能學到東西的人。爭論本身不是目的,讓雙方都把話講清楚才是。
  • 判斷自己是不是碰到了認知天花板,可以先問一句:我是在計算上做不到,還是在理解上做不到?這兩件事完全不同。威滕看不見上百維空間,但他能理解它。

最後留一個卡羅爾式的態度。他說,在所有讓他睡不著的擔憂裡,人類理性不夠用這一條排名很靠後。500年前最聰明的人也以為自己快到頭了,結果他們連經典力學都還沒有。

我們大機率也還沒到頭。

文稿由本站用語音識別模型(基於官方釋出音訊)機器轉寫,可能有識別錯誤,人名與數字請以音訊為準。
[00:00:00] The following is a conversation with Sean Carroll, part two, the second time we've spoken on the podcast, you can get the link to the first time in the description. This time we focus on quantum mechanics and the many worlds interpretation that he details elegantly in his new book titled Something Deeply Hidden. I own and enjoy both the e-book and audiobook versions of it. Listening to Sean read about entanglement complimentarity and the emergence of space time reminds me of Bob Ross teaching the world how to paint and his old television show. [00:00:35] If you don't know who Bob Ross is, you're truly missing out. Look him up. He'll make you fall in love with painting. Sean Carroll is the Bob Ross of Theoretical Physics. He's the author of several popular books, a host of a great podcast called Mindscape and is a theoretical physicist at Caltech and the Santa Fe Institute specializing in quantum mechanics or of time, cosmology and gravitation. This is the Artificial Intelligence Podcast. If you enjoy, subscribe on YouTube, give it five stars on iTunes, supported on Patrón or simply connect with me on Twitter. [00:01:14] Elex Friedman spelled F.R. Idi Amin. And now here's my conversation with Sean Carroll. Isaac Newton developed what we now call classical mechanics that you describe very nicely in your new book, as you do with a lot of basic concepts in physics. So was classical mechanics. I can throw a rock and can predict the trajectory of that rock's flight. [00:01:58] But if we could put ourselves back into Newton's time, his theories work to predict things. But as I understand, he himself thought that they were the interpretations of those predictions were absurd. And perhaps he just said it for religious reasons and so on. [00:02:16] But in particular, sort of a world of interaction with our contact. So action at a distance, it didn't make sense to him in a sort of a human interpretation level. Does it make sense to you that things can affect other things at a distance? It does, but you know that so that was one of Newton's worries, you're actually right in a slightly different way about the religious worries. He he was smart enough. This is off the topic, but still fascinating. [00:02:45] Newton almost invented chaos theory. As soon as he invented classical mechanics, he realized that in the solar system. So he was able to explain how planets move around the sun. [00:02:56] But typically you would describe the orbit of the Earth, ignoring the effects of Jupiter and Saturn and so forth, just doing the Earth in the sun. [00:03:03] He he kind of knew, even though he couldn't do the math, that if you included the effects of Jupiter and Saturn, the other planets, the solar system would be unstable, like the orbits of the planets would get out of whack. So he thought that God would intervene occasionally to sort of move the planets back into orbit, which is how you could only way you could explain how they were there, presumably forever. But the worry about classical mechanics were a little bit different. [00:03:25] The worry about gravity in particular wasn't a worry about classical mechanics or about gravity. How in the world does the Earth know that there's something called the sun 93 million miles away that is exerting gravitational force on it? [00:03:37] And he said he literally said, you know, I leave that for future generations to think about because I don't know what the answer is. [00:03:43] And in fact, the people underemphasized this, but future generations figured it out. Peerce among the class in circa 1800 showed that you could rewrite Newtonian gravity as a field theory. So instead of just talking about the force due to gravity, you can talk about the gravitational field or the gravitational potential field, and then there's no action at a distance. [00:04:05] It's exactly the same theory empirically. It makes exactly the same predictions. But what's happening is instead of the sun just reaching out across the void, there is a gravitational field in between the sun, in the earth that obeys an equation, lipless equation cleverly enough, and that tells us exactly what the field does. [00:04:22] So even in Newtonian gravity, you don't need action at a distance. Now, what many people say is that Einstein solved this problem because he invented general relativity and general relativity. There's certainly a field in between the Earth and the sun, but also there's the speed of light as a limit in La Plaza's theory, which was exactly Newton's theory. Just in a different mathematical language, there could still be instantaneous action across the universe, whereas in general relativity, if you shake something here, it's gravitational impulse radiates out at the speed of light. [00:04:53] We call that a gravitational wave and we can detect those. [00:04:56] So but I really it rubs me the wrong way to think that we should presume the answer should look one way or the other, like if it turned out that there was action at a distance in physics and that is the best way to describe things that I would do it that way. It's actually a very deep question, because when we don't know what the right laws of physics are, when we're guessing at them, when we're hypothesizing at what they might be, we are often guided by our intuitions about what they should be. [00:05:24] I mean, Einstein famously was very guided by his intuitions and he did not like the idea of action at a distance. We don't know whether he was right or not, it depends on your interpretation of quantum mechanics and it depends on even how you talk about quantum mechanics within any one interpretation. [00:05:41] If you see every forces of field or any other interpretation of action at a distance is just stepping back to sort of caveman thinking. Do you really can you really sort of understand what it means for a force to be a field that's everywhere? So if you look at gravity, like, what do you think about? I think so. Is this something that you've been conditioned? By society to think that to map the fact that science is extremely well predictive of something to believing that you actually understand it, like you can intuitively do as the degree that human beings can understand anything, that you actually understand it. [00:06:30] Are you just trusting the beauty and the power of the predictive power of science? [00:06:36] That depends on what you mean by this idea of truly understanding. Right. Right. [00:06:42] You know, I mean, can I fully understand Fermat's last theorem? [00:06:46] You know, it's easy to state it, but do I really appreciate what it means for incredibly large numbers? Right. I think yes. I think I do understand it. But like, if you want to just push people on. Well, but your intuition doesn't go to the places where Andrew Wiles needed to go to prove Fermat's last theorem. [00:07:05] And I can say fine, but I still think I understand that theorem. And likewise, I think that I do have a pretty good intuitive understanding of fields pervading spacetime, whether it's the gravitational field or the electromagnetic field or whatever the Higgs field. [00:07:20] Of course, one's intuition gets worse and worse as you get trickier in quantum field theory and all sorts of new phenomena that come up in quantum field theory. So our intuitions aren't perfect. But I think it's also OK to say that our intuitions get trained like, you know, I have different intuitions now than I had when I was a baby. That's OK. That's not an intuition is not necessarily intrinsic to who we are. We can we can train it a little bit. [00:07:44] So that's where I'm going to bring in Noam Chomsky for a second who thinks that our cognitive abilities are sort of evolved through time. And so they're biologically constrained. And so there's a clear limit, as he puts it, to our cognitive abilities. And it's a very harsh limit. But you actually kind of said something interesting in nature versus nurture thing here is we can train our intuitions to sort of build up the cognitive muscles, to be able to understand some of these tricky concepts. [00:08:17] Did you do you think there's limits to our understanding that's deeply rooted, hardcoded into our biology that we can't overcome? [00:08:27] There could be limits to things like our ability to visualize. OK, but when someone like Ed Witten proves the theorem about hundred dimensional mathematical spaces, he's not visualizing it. He's doing the math. That doesn't stop him from understanding the result. I think and I would love to understand this better, but my rough feeling, which is not very educated, is that, you know, there's some threshold that one crosses in abstraction when one becomes kind of like a Turing machine, right. [00:08:58] One has the ability to contain in one's brain logical, formal symbolic structures and manipulate them. And that's a leap that we can make as human beings that that dogs and cats haven't made. [00:09:11] And once you get there, I'm not sure that there are any limits to our ability to understand the scientific world at all. [00:09:19] Maybe there are. There's certainly limits in our ability to calculate things. Right. You know, people are not very good at taking cube roots of million digit numbers in their head. But that's not a limit of understanding. It's certainly not a limiting principle. [00:09:33] So, of course, as a human, you would say that doesn't feel to be limited to our understanding, but sort of. [00:09:41] Have you thought that the universe is actually a lot simpler than it appears to us and we just will never be able to get outside of our OK, so us our cognitive abilities, combined with our mathematical prowess and whatever kind of experimental simulation devices we can put together is there are limits to that. [00:10:07] Is is it possible there's limits to that? [00:10:10] Well, of course it's possible. [00:10:12] But the problem with that, is there any good reason to think that we're anywhere close to the limits is a harder question. Look, imagine asking this question 500 years ago to the world's greatest thinkers, right? Like are approaching the limits of our ability to understand the natural world. And by definition, there are questions about the natural world that are most interesting to us that are the ones we don't yet understand. So there's always we're always faced with these puzzles. [00:10:39] We don't yet know. And I don't know what they would have said five hundred years ago, but they didn't even know about classical mechanics, much less quantum mechanics. [00:10:46] So we know that they were nowhere close to how well they could do. Right. They could do enormously better than they were doing at the time. I see no reason why the same thing isn't true for us today. So of all the worries that keep me awake at night, the human minds inability to rationally comprehend the world is low on the list. [00:11:06] Well, but so one interesting philosophical point and quantum mechanics bring up is the way you talk about the distinction between the world as it is and the world as we observe it. Mm hmm. [00:11:19] So staying at the human level for a second, how big is the gap between what our perception system allows us to see and the world as it is outside our mind's eye? Sort of. [00:11:32] Sort of not at the quantum mechanical level, but as just these particular tools we have, which is the few senses and cognitive abilities to process those senses? [00:11:43] Well, that last phrase, having the cognitive abilities to process them carries a lot, right? I mean, there is our sort of intuitive understanding of the world. You don't need to teach people about gravity for them to know that apples fall from trees. Right. That's something that we figure out pretty quickly. Object permanence, things like that. The three dimensionality of space, even if we don't have the mathematical language to say that, we kind of know that it's true. [00:12:09] On the other hand, no one opens their eyes and sees atoms or molecules or cells for that matter. Forget about quantum mechanics. [00:12:17] So but we got there. We got to understanding that there are atoms and cells using the combination of our senses and our cognitive capacities. [00:12:28] So adding the ability of our cognitive capacities to our senses is adding an enormous amount. And I don't think it is a hard and fast boundary. You know, if you believe in cells, if you believe we understand those and there's no reason to believe, we can't believe in quantum mechanics just as well. [00:12:46] What to you is the most beautiful idea in physics? Conservation of momentum, can you elaborate? Yeah, if you were Aristotle when Aristotle wrote his book on physics, he made the following very obvious point. [00:13:02] We're on video here so people can see this. So if I push the bottle, let me cover this bottle so we do not have a mess. But OK, so I push the bottle, it moves. And if I stop pushing, it stops moving. Yes. And this is this kind of thing is repeated a large number of times all over the place. If you don't keep pushing things, they stop moving. This is a indisputably true fact about our everyday environment, OK? [00:13:26] And for Aristotle, this blew up into a whole picture of the world in which things had natures and teleology and they had places they wanted to be. And when you were pushing them, you were moving them away from where they wanted to be and they would return and stuff like that. [00:13:41] And it took a thousand years or fifteen hundred years for people to say, actually, if it weren't for things like dissipation and air resistance and friction and so forth, the natural thing is for things to move forever in a straight line. There's a constant velocity, right. Conservation of momentum. [00:14:01] And that is the reason why I think that's the most beautiful idea in physics, is because it shifts us from a view of nature's and teleology to a view of patterns in the world. So when you were Aristotle, you needed to talk a vocabulary of why is this happening? Was the purpose of it was the cause, et cetera. Because, you know, its nature does or does not want to do that. Whereas once you believe in conservation momentum, things just happen. [00:14:30] They they just follow the pattern you give me. You have this demon ultimately, right. You give me the state of the world today. I can predict what's going to do in the future. I can predict where it was in the past. [00:14:40] It's impersonal and it's also instantaneous. It's not directed toward any future goals. It's just doing what it does, given the current state of the universe that I think even more than either classical mechanics or quantum mechanics, that is the profound deep insight that gets modern science off the ground. You don't need natures and purposes and goals. You just need some patterns. [00:15:03] Since the first moment in our understanding of the way the universe works, where you branch from the intuitive physical space to kind of the space of ideas. And also the other point you said, which is conveniently most of the interesting ideas are acting in the moment. You don't need to know the history of time or the future. [00:15:26] Then, of course, this took a long time to get there, right? I mean, the conservation momentum itself took hundreds of years. It's weird because, like, someone would say something interesting and then the next interesting thing would be said like one hundred and fifty or two hundred years later. Right. They weren't even talking to each other. They were reading each other's books. And probably the first person to directly say that in outer space, in the vacuum projectile would move at a constant velocity was of Azana, even Seina in the Persian golden age circa one thousand. [00:15:55] And he didn't like the idea. He used that just like Schrodinger used Schrodinger's cat to say, surely you don't believe that, right? Even Senior was saying, surely don't believe there really is a vacuum, because if there was really a vacuum, things could keep moving forever. Right. But still, he got right. The idea that there was this conservation of something impetus or Myal, he would call it, and that's five hundred years. [00:16:17] Six hundred, six hundred years before classical mechanics and Isaac Newton. So, you know, Galileo played a big role in this, but he didn't exactly get it right. And so it just takes a long time for this to sink in because it is so against our everyday experience. [00:16:30] Do you think it was a big leap, a brave or a difficult leap of sort of math and science to be able to say that momentum is conserved? I do you know, I think it's an example of human reason in action, you know, even Aristotle knew that his theory had issues because you could fire an arrow and would go a long way before it stopped. So if his theory was things just automatically stop, what's going on? And he had this elaborate story, I don't know if you've heard the story, but the arrow would push the air in front of it away and the molecules of air would run around the back of the arrow and push it against anyone. [00:17:11] Reading this is going like, really, that's that's what you thought. But it was that kind of thought experiment that ultimately got people to say, like, actually, no, if it weren't for the air molecules at all, there would just go on by itself. And it's always this give and take between thought and experience back and forth. Right. Theory and experiment, we would say today. [00:17:30] Another big question that I think comes up certainly with quantum mechanics is what's the difference between math and physics? To you? [00:17:42] To me, you know, very, very roughly, math is about the logical structure of all possible worlds, and physics is about our actual world. [00:17:52] And it just feels like our actual world is a gray area when you start talking about interpretations of quantum mechanics or no, I'm certainly using the word world in the broadest sense, all of reality. [00:18:05] So I think the reality is specific. I don't think that there's every possible thing going on in reality. I think there are rules, whether it's the Schrodinger equation or whatever. So I think I think that there's a sensible notion of the set of all possible worlds. And we live in one of them. The world that we're talking about might be a multiverse, might be many worlds of quantum mechanics, might be much bigger than the world of our everyday experience. [00:18:27] But it's still one physically contiguous world in some sense. [00:18:32] But so if you look at the overlap of math and physics, it feels like one physics tries to reach for understanding of our world. [00:18:44] It uses the tools of math to sort of reach beyond the limit of our current understanding. [00:18:51] What do you make of that process of sort of using math to so you start maybe with intuition or you might start with the math and then build up an intuition or but this kind of reaching into the darkness, into the mystery of the world with math? [00:19:07] Well, I think I would put it a little bit differently. I think we we have theories, theories of the physical world, which we then extrapolate and ask, you know, what do we conclude if we take these seriously well beyond where we've actually tested them. It is separately true that math is really, really useful when we construct physical theories. And, you know, famously, Eugene Wigner asked about the unreasonable success of mathematics and physics. I think that's a little bit wrong because anything that could happen, any other theory of physics that wasn't the real world, but some other world, you could always describe it mathematically. [00:19:43] It's just that it might be a mess. The surprising thing is not that math works, but that the math is so simple and easy that you can write it down on a T-shirt, right? I mean, that's what is amazing. That's an enormous compression of information that seems to be valid in the real world. So that's an interesting fact about our world, which maybe we could hope to explain or just take as a brute fact. [00:20:06] I don't know. But once you have that, you know, there's this indelible relationship between math and physics. But but philosophically, I do want to separate them. What we what we extrapolate we don't extrapolate math because there's a whole bunch of wrong math, you know, that doesn't apply to our world. Right. We extrapolate the physical theory that we best think explains our world. [00:20:27] Again, an unanswerable question. [00:20:29] Why do you think our world is so easily compressible into beautiful equations? Yeah, I mean, like I just hinted at, I don't know if there's an answer to that question. [00:20:41] There could be what would an answer look like? Well, an answer could look like if you showed that there was something about our world that maximized something. You know, the the the mean of the simplicity in the powerfulness of the laws of physics or you know what, maybe we're just generic, maybe in the set of all possible worlds. [00:21:00] This is what the world would look like. Right? [00:21:02] Like, I don't really know. I tend to think not. I tend to think that there is something specific and rock bottom about the facts of our world that don't have further explanation, like the fact that the world exists at all. And furthermore, the specific laws of physics that we have, I think that in some sense we're just going to at some level we're going to say, and that's how it is. And, you know, we can't explain anything more. [00:21:24] I don't know how if we're anywhere close to that right now, but that seems possible to me. [00:21:29] And speaking of rock bottom, one of the things in your book kind of reminded me of revealed to me is that what's fundamental and what's emergent, it just feels like I don't even know anymore what's fundamental in in physics. If there's anything it feels like everything, especially quantum mechanics, is revealing to us. [00:21:50] Is that most interesting things that I would as a as a limited human would think are fundamental art can actually be explained as emergent from the the more deeper laws. [00:22:06] I mean, we don't know. Of course, you had to get that on the table. We don't know what is fundamental. We do know we do have reason to say that certain things are more fundamental than others. Right. Atoms and molecules are more fundamental than cells and organs. Quantum fields are more fundamental than atoms and molecules. We don't know if that ever bottoms out. I do think that there's sensible ways to think about this. The if you if you describe something like this table as a table, it has a height and a width and it's made up of certain material and has a certain solidity and weight and so forth. [00:22:39] That's a very useful description as far as it goes. There's a whole nother description at this table in terms of a whole collection of atoms strung together in certain ways, the language of the atom. [00:22:50] Is more comprehensive in the language of the table, you could break apart the table, smashed to pieces, still talk about it as Adams, but you could no longer talk about it as a table, right? So I think at this comprehensiveness, the domain of validity of a theory gets broader and broader as the theory gets more and more fundamental. [00:23:10] So what do you think Newton would say? Maybe write in the book review? [00:23:16] If you read your latest book on quantum mechanics, something deeply hidden, it would take a long time for him to think that any of this was making any sense. [00:23:25] You catch him up pretty quick in the beginning. Yeah. You give him a shout out at the beginning. That's right. [00:23:30] I mean, he is the man I'm happy to say that Newton was the greatest scientists who ever lived. I mean, he invented calculus in his spare time, which would have made it the greatest mathematician just all by himself. Right. That one thing. [00:23:42] But, of course, you know, it's funny because Newton was in some sense still a premodern thinker. Rocky Kolbe, who is a cosmologist at the University of Chicago, said that, you know, Galileo, even though he came before Newton, was a more modern thinker than Newton was like, if you got Galileo and brought him to the present day, you take him six months to catch up. And then he'd be in your office telling you what your most recent paper was wrong. [00:24:07] Whereas Newton just thought in this kind of more mystical way, you know, he wrote a lot more about the Bible and alchemy than he ever did about physics. And but he's also more brilliant than anybody else and way more mathematically astute than Galileo. So I really don't know. You know, he he might have he might just say, like, give me the textbooks, leave me alone for a few months and then be caught up. But he might have had mental blocks against against seeing the world in this way. [00:24:37] I really don't know or perhaps find an interesting mystical interpretation of quantum mechanics. Very possible. Yeah. [00:24:43] Is there any other scientists or philosophers through history that you would like to know their opinion of your book? That's a that's a good question. [00:24:54] I mean, Einstein is the obvious one, right? All I mean, he was not that long ago. But you can speculate at the end of my book about what is it Penny would be. [00:25:01] I am curious as to, you know, what about older philosophers like Hume or can't write like what would they have thought? Or Aristotle, you know, what would they thought about modern physics? [00:25:12] Because they do in philosophy, your predilections end up playing a much bigger role in your ultimate conclusions because you're not as tied down by what the data is. [00:25:23] In physics, you know, physics is lucky because we can't stray too far off the reservation as long as we're trying to explain the world that we actually see in our telescopes and microscopes. [00:25:33] But it's just not fair to play that game because the people we're thinking about didn't know a whole bunch of things that we know. Right. Like we lived through a lot that they didn't live through. So by the time we got them caught up, they'd be different people. [00:25:49] So let me ask a bunch of basic questions. I think it would be interesting, useful for people who are not familiar, but even for people who are extremely well familiar. Let's start with what is quantum mechanics? [00:26:04] Quantum mechanics is the paradigm of physics that came into being in the early part of the 20th century that replaced classical mechanics and it replaced classical mechanics in a weird way that we're still coming to terms with. So in classical mechanics, you have an object, it has a location, has a velocity. And if you know the location of velocity of everything in the world, you can say, well, everything's going to do. [00:26:27] Quantum mechanics has an aspect of it that is kind of on the same lines. [00:26:32] There's something called the quantum state or the wavefunction, and there's an equation governing what the quantum state does. So it's very much like classical mechanics. The way function is different. It's sort of a wave. It's a vector in a huge dimensional vector space rather than a position and a velocity. But OK, that's a detail. And the equation is the Schrodinger equation, not Newton's laws. But OK, again, a detail where quantum mechanics really becomes weird and different is that there's a whole nother set of rules in our textbook formulation of quantum mechanics. [00:27:02] In addition to saying that there's a quantum state and it evolves in time. [00:27:06] And all these new rules have to do with what happens when you look at the system, when you observe it, when you measure it. [00:27:12] In classical mechanics, there were no rules about observing. [00:27:15] You just look at it and you see what's going on. That that was that right. In quantum mechanics, the way we teach it, there's something profoundly fundamental about the act of measurement or observation in the system dramatically changes its state, even though it has a wave function like the electron in an atom is not orbiting in a circle, is sort of spread out in the cloud. [00:27:36] When you look at it, you don't see that cloud. When you look at it, it looks like a particle with a location. So it dramatically changes its state right away and the effects of that change can be instantly seen. And what the electron does next. [00:27:49] So that's that. Again, we need to be careful because we don't agree on what quantum mechanics says. [00:27:55] So that's why I need to say, like in the textbook view that are right. [00:27:58] But in the textbook view, quantum mechanics, unlike any other theory of physics places, gives a fundamental role to the act of measurement. [00:28:08] So maybe even more basic, what is an atom and what is an electron? [00:28:14] Sure, this all came together in a few years around the turn of the last century, right around the year 1900. Adams predated then, of course, the word Adam goes back to the ancient Greeks, but it was the chemists in the eighteen hundreds that really first got experimental evidence for atoms. They realized, you know, that there were two different types of tin oxide. And in these two different types of tin oxide, there was exactly twice as much oxygen in one type as the other. [00:28:44] And like, why is that? Why is it was it never one point five times as much? Right. And so Dalton said, well, it's because there are ten atoms and oxygen atoms and one form of tin oxide is one atom of ten and one atom of oxygen, and the other is one out of 10 and two atoms of oxygen. And on the basis of speculation, a theory, right. A hypothesis. But then on the basis of that, you make other predictions. [00:29:08] And the chemists became quickly convinced that atoms were real. The physicist took a lot longer to catch on, but eventually they did. And I mean, Boltzmann, who believed in atoms, was, God, you had a really tough time his whole life because he worked in Germany where atoms were not popular. They were popular in England, but not in Germany. [00:29:26] And there in general, the idea of atoms is the most the smallest building block of the universe for them. That's the kind of how the Greek idea. But the chemists, the eighteen hundreds jumped the gun a little bit. So these days in Atom is the smallest building block of a chemical element. Right. Hydrogen, 10, oxygen, carbon, whatever. But we know that atoms can be broken up further than that. And that's what physicists discovered in the early nineteen hundreds, Rutherford especially, and his colleagues. [00:29:57] So the atom that we think about now, the cartoon is that picture you you always seen of a little nucleus and then electrons orbiting it like a little solar system. And we now know the nucleus is made of protons and neutrons. So the weight of the atom, the mass is almost all in its nucleus, protons and neutrons or something like eight hundred times as heavy as electrons are. [00:30:20] Electrons are much lighter, but because they're lighter, they give all the life to the atoms. So in atoms, get together, combine chemically. When electricity flows through a system, it's all the electrons that are doing all the work. [00:30:33] And where quantum mechanics steps in, as you mentioned, with position of velocity, with classical mechanics and quantum mechanics, is modeling the behavior of the electron. I mean, you can model the behavior of anything but the electron because that's where the fun is. [00:30:49] The electron was the biggest challenge right from the start. Yeah. So what's the wavefunction? You said it's an interesting detail. Yeah. [00:30:56] But in any interpretation, what is the wavefunction and quantum mechanics? [00:31:02] Well, you know, we had this idea from Rutherford that atoms look like little solar systems, but people very quickly realize that can't possibly be right, because if an electron is orbiting in a circle, it will give off light. All the light that we have in this room comes from electrons zooming up and down and wiggling. And that's what electromagnetic waves are. And you can calculate how long would it take for the electron just to spiral into the nucleus? [00:31:25] And the answer is ten to the minus 11 seconds. OK, a hundred billionth of a second. So that's not right. [00:31:31] Meanwhile, people had realized that light, which we understood from the eighteen hundreds was a wave, had properties that were similar to that of particles. Right. [00:31:41] This is Einstein and plonk and stuff like that. So if something that we agree was a wave had particle like properties, then maybe something that we think is a particle. The electron has wavelike properties. [00:31:54] Right. And so a bunch of people eventually came to the conclusion, don't think about the electron is a little point particle orbiting like a solar system. [00:32:04] Think of it as a wave that is spread out. They cleverly gave this the name the wave function, which is the dopiest name in the world for one of the most profound things in the universe. There's literally, you know, a number at every point in space, which is the value of the electrons wavefunction at that point. [00:32:22] And there's only there's only one way function that, yeah, they eventually figured that out. That took longer. But when you have two electrons, you do not have a wavefunction for electron one in a wavefunction for electron two. You have one combined wavefunction for both of them. And indeed, as you say, there's only one wavefunction for the entire universe at once. [00:32:43] And that's where this beautiful dance. Can you say what is entanglement? It seems one of the most fundamental ideas of quantum mechanics. [00:32:52] Let's temporarily buy into the textbook interpretation of quantum mechanics. And what that says is that this wave function, so it's very small outside the atom, very big in the atom, basically the wavefunction, you take it and you square it, you square the number that gives you the probability of observing the system at that location. So if you say that for two electrons, there's only one wave function and that wave function gives you the probability of observing both electrons at once doing something, OK, so maybe. [00:33:21] The electron can be here, here, here, here, and the other electron can also be there, but we have a wavefunction set up where we don't know where either electron is going to be seen, but we know they'll both be seen in the same place. OK, so we don't know exactly what we're going to see for either electron, but there's entanglement between the two of them. There's a sort of conditional statement. If we see one in one location, then we know the other one's going to be doing a certain thing. [00:33:47] So that's a feature of quantum mechanics that is nowhere to be found in classical mechanics and classical mechanics. There's no way I can say, well, I don't know where either one of these particles is, but if I know if I find out where this one is, then I know where the other one is. That just never happens. They're truly separate. [00:34:00] And in general, it feels like if you think of a wavefunction, like as a dance floor, it seems like entanglement is strongest between things that are dancing together closest. So there's a there's a closeness that's important. Well, that's not that. That's another step. We have to be careful here, because in principle, if you if you talk about the entanglement of two electrons, for example. They can be totally entangled or totally untangled, no matter where they are in the universe, there's no relationship between the amount of entanglement and the distance between two electrons. [00:34:33] But we now know that the reality of our best way of understanding the world is through quantum fields, not through particles. So even the electron, not just gravity and electromagnetism, but even the electron and the quarks and so forth are really vibrations in quantum fields. So even empty space is full of vibrating quantum fields, and those quantum fields in empty space are entangled with each other in exactly the way you just said. If they're nearby, if you have like two vibrating quantum fields that are nearby, then they will be highly entangled. [00:35:05] If they're far away, they will not be entangled. [00:35:07] So what do quantum fields in a vacuum look like? Empty space, just like empty space is as empty as it can be. But there's still a field. It's just. Yeah, it what is nothing? [00:35:19] Just like right here at this location in space, there's a gravitational field which I can detect by dropping something inside. I don't see it, but there it is. [00:35:30] So we've got a little bit of idea of entanglement now. What is Hilbert space and Euclidean space? [00:35:42] Yeah, you know, I think that people are very welcome to go through their lives not knowing what Hilbert space is. But if you if you dig into a little bit more into quantum mechanics, it becomes necessary. You know, the English language was invented long before quantum mechanics or various forms of higher mathematics were invented. [00:35:58] So we use the word space to mean different things. Of course, most of us think of space as this three dimensional world in which we live. I mean, some of us just think of it as outer space, OK? But space around us gives us the three dimensional location of things and objects. But mathematicians use any generic abstract collection of elements as a space, a space of possibilities, you know, momentum, space, et cetera. So Hilbert space is the space of all possible quantum wave functions, either for the universe or for some specific system. [00:36:33] And it could be an infinite dimensional space or it could be just really, really large dimensional but finite. We don't know because we don't know the final theory of everything. But this abstract Hilbert space is really, really, really big and has no immediate connection to the three dimensional space in which we live. What do dimensions in Hilbert space mean? [00:36:52] You know, it's just a way of mathematically representing how much information is contained in the state of the system. How many numbers do you have to give me to specify what the thing is doing? So in classical mechanics, I give you the location of something by giving you three numbers right up, down, X, Y, Z coordinates. But then I might want to give you its entire state physical state, which means both its position and also its velocity. [00:37:19] The velocity also has three components. So its state lives in something called phase space, which is six dimensional, three dimensions of position, three dimensions of velocity. [00:37:29] And then if it also has an orientation in space, that's another three dimensions and so forth. So as you describe more and more information about the system, you have an abstract mathematical space that is more and more numbers that you need to give. And each one of those numbers corresponds to a dimension in that space. [00:37:46] So in terms of that amount of information, what is entropy, this mystical word that's overused in math and physics but has a very specific meaning in this context? [00:37:59] Sadly, it has more than one very specific meaning. This is this is reason why it is hard. Entropy means different things even to different physicists. But one way of thinking about it is a measure of how much we don't know about the state of a system. Right. So if I have a bottle of water molecules and I know that, OK, there's a certain number of water molecules, I could weigh it right and figure out I know the volume of it and I know the temperature and pressure and things like that. [00:38:24] I certainly don't know the exact position and velocity of every water molecule. [00:38:28] Right. So there's a certain amount of information I know certain about that. I don't know. That is that is part of the complete state of the system. And that's what the entropy characterizes, how much unknown information there is. The difference between what I do know about the system and is full, exact microscopic state. [00:38:45] So when we try to describe a quantum mechanical system, is it infinite or finite, but very large? [00:38:54] Yeah, we don't know that. It depends on the system. You know, it's easy to mathematically write down a system that would have a potentially infinite entropy and infinite dimensional Hilbert space. So let's let's go back a little bit. We said that the Hilbert space was the space in which quantum wave functions lived for different systems. That will be different sizes. They could be infinite or finite. [00:39:15] So that's the number of numbers, the number of pieces of information you could potentially give me about the system. So the bigger Hilbert space is, the bigger the entropy of that system could be. Depending on what I know about it. If I don't know anything about it, then, you know, has a huge entropy. Right. [00:39:32] But only up to the size of its Hilbert space. So we don't know in in the real physical world whether or not this region of space that contains that water bottle has potentially an infinite entropy or just a finite entropy. We have we have different arguments on different sides. [00:39:48] So if it's infinite, how do you think about infinity? Is this something you can call your cognitive abilities are able to process or is it just a mathematical tool? [00:40:01] It's somewhere in between, right? I mean, we can say things about it. We can use mathematical tools to manipulate infinity very, very accurately. You can define what we mean, you know, for any number N there's a number bigger than it. So there's no biggest number. Right. So there's something called the total number of all numbers. That's infinite. But it is hard to wrap your brain around that. And I think that gives people pause because we talk about infinity as if it's a number, but it has plenty of properties that real numbers don't have. [00:40:29] You know, if you multiply infinity by two, you get infinity again. Right. That's a little bit different than what we're used to. OK, but are you comfortable with the idea that in thinking of what the real world actually is, that infinity could be part of that world? Are you comfortable that a world in some dimension and are comfortable with lots of things? [00:40:50] I mean, you know, I don't want my level of comfort to affect. [00:40:56] What I think about the world, you know, I'm pretty open minded about what the world could be at the fundamental level. Yeah, but infinity is a is a tricky one. It's not almost a question of comfort. [00:41:07] It's a question of is it an overreach of our intuitions or it could be a convenient almost like when you add a constant to an equation just because it'll help. It just feels like it's useful to at least be able to imagine a concept not directly, but in some kind of way, that this feels like it's a description of the real world. [00:41:31] Think of it this way. There's only three numbers that are simple. [00:41:36] There's zero, there's one and there's infinity. [00:41:41] A number like three hundred and eighteen. It's just bizarre like that that you need a lot of bits to give me what that number is. Yeah, but zero and one infinity. Like once you have three hundred things you might as well have infinity things. Right. Otherwise you have to say when to stop making the thing. That's right. So there's a sense in which infinity is a very natural number of things to exist. [00:42:02] I was never comfortable with infinity because it's just such a it was too good to be true because in math it just helps make things work out. [00:42:12] When things get very it's when things get very large, close to infinity, things seem to work out nicely. It's kind of like because my my deepest passion is probably psychology and I'm uncomfortable. [00:42:26] How in the average the the beauty of the very the how much we vary is lost in that same kind of sense. Infinity seems like a convenient way to erase the details. [00:42:41] But the thing about infinity is it seems to pop up whether we like it or not. [00:42:45] Right. Right. Like you're trying to be a computer scientist. You ask yourself, well, how long will it take this program to run? And you realize, well, some of them, the answer is infinitely long. It's not because you tried to get there. You wrote a five line computer program. It doesn't halt. [00:43:00] So coming back to the textbook definition of quantum mechanics, this idea that I don't think we talked about, can you this is one of the most interesting philosophical points. We've talked at the human level, but at the at the physics level that at least the textbook definition of quantum mechanics separates what is observed and what is the real one. How does that make you feel? And and and to what does it then mean to observe something? And why is it different than what is real? [00:43:37] Yeah, you know, my personal feelings such as it is, is that things like measurement and observers and stuff like that are not going to play a fundamental role in the ultimate laws of physics. But my feeling that way is because so far that's where all the evidence has been pointing. [00:43:55] I could be wrong. And there's certainly a sense in which it would be infinitely cool if somehow observation or mental computation did play a fundamental role in the nature of reality. But I don't think so, and I don't see any evidence for it. So I'm not spending a lot of time worrying about that possibility. [00:44:15] So what do you do about the fact that in the textbook interpretation of quantum mechanics, this idea of measurement or looking at things seems to play an important role? Well, you you come up with better interpretations of quantum mechanics and there are several alternatives. [00:44:29] My favorite is the many worlds interpretation, which says two things. Number one, you, the observer, are just a quantum system. Like anything else. There's nothing special about you don't get so proud of yourself. You know, you're just a bunch of atoms. You have a wave function. You obey the Schrodinger equation like everything else. And number two, when you think you're measuring something or observing something, what's really happening is you're becoming entangled with that thing. [00:44:57] So when you think there's a wave function for the electron, it's all spread out. But you look at it and you only see it in one location. What's really happening is that there's still the wave function, the electron and all those locations, but now it's entangled with the wave function of you in the following way. There's part of the wave function that says the electron was here and you think you saw it there, the electron was there and you think you saw it there. [00:45:19] The electron was over there and you think you saw it there, et cetera. [00:45:22] So and all of those different parts of the wave function, once they come into being no longer talk to each other, they no longer interact or influence each other. [00:45:31] It's as if they are separate worlds. So this was the invention of Hugh Everett, the third, who was a graduate student at Princeton in the 1950s. And he said basically, look, you don't need all these extra rules about looking at things. Just listen to what the Schrodinger equation is telling you. It's telling you that you have a wavefunction that you become entangled and that the different versions of you no longer talk to each other. [00:45:55] So. Just accept it, it's just he did therapy more than anything else, you know, he said like, it's OK, you know, you don't need all these extra rules or you need to do is believe the Schrodinger equation. The cost is there's a whole bunch of extra worlds out there. [00:46:07] So other worlds being created, whether there's an observer or not, the worlds are created any time a quantum system that's in a superposition becomes entangled with the outside world. [00:46:21] What's the outside world? It depends. Let's back up whatever it really says, what his theory is, is there's a wavefunction of the universe and it obeys the Schrodinger equation all the time. That's it. That's the full theory right there, OK. [00:46:37] The question all of the work is how in the world do you map that theory onto reality, onto what we observe? [00:46:45] Right. So part of it is carving up the wavefunction into these separate worlds, saying, look, look, it describes a whole bunch of things that don't interact with each other. Let's call them separate worlds. Another part is distinguishing between systems and their environments. And the environment is basically all the degrees of freedom, all the things going on in the world that you don't keep track of. So, again, in the bottle of water, I might keep track of the total amount of water and the volume. [00:47:11] I don't keep track of the individual positions and velocities. I don't keep track of all the photons or the air molecules in this room. So that's the outside world. The outside world is all the parts of the universe that you're not keeping track of when you're asking about the behavior of some subsystem of it. [00:47:28] So how many worlds are there going to know that one? [00:47:33] Either there could be an infinite number, there could be only a finite number, but it's a big number one way or the other. [00:47:39] It's just a very, very big number. In one of the talks, somebody asked, well, if it's a. If it's finite. So actually, I'm not sure exactly the logic you used to drive this, but is there going to be, you know, overlap a duplicate world that you return to? So you've mentioned and I'd love if you can elaborate on sort of idea that it's possible that there's some kind of equilibrium that these splitting worlds arrive at and then maybe over time, maybe somehow connected to entropy, you get a large number of worlds that are very similar to each other. [00:48:22] Yeah. So this question of whether or not Hilbert space is finite or infinite dimensional is actually secretly connected to gravity and cosmology. This is the part that we're still struggling to understand right now. But we discovered back in nineteen ninety eight that our universe is accelerating. And what that means if it continues, which we think it probably will, but we're not sure. But if it does, that means there's a horizon around us there. There's because the universe not only expanding but expanding faster and faster things can get so far away from us that from our perspective, it looks like they're moving away faster than the speed of light. [00:48:58] You'll never see them again. So there's literally a horizon around us in that horizon approaches some fixed distance away from us. And you can then argue that within that horizon, there's only a finite number of things that can possibly happen. The finite dimensional Hilbert space. In fact, we even have a guess for what the dimensionality is. It's ten to the power of ten to the power of one hundred twenty two. [00:49:21] That's a very large number. Yes. Just to compare, the age of the universe is something like 10 of the 14 seconds, 10 of the 17 or 18 seconds, maybe the number of particles in the universe is ten of the 88. But the number of dimensions of Hilbert space is ten to the ten to the one hundred and twenty two. [00:49:38] So that's just crazy because if that story is right, that in our observable horizon there's only a finite dimensional Hilbert space, then this idea of branching, of the wavefunction of the universe into multiple distinct separate branches has to reach a limit at some time. Once you branch that many times, you've run out of room in Hilbert space. [00:49:58] And roughly speaking, that corresponds to the universe just expanding and emptying out and cooling off and entering a phase where it's just empty space literally forever. [00:50:10] What's the difference between splitting and copying, do you think, in terms of a lot of this is an interpretation that that helps us sort of model the world so perhaps shouldn't be thought of as like, you know, philosophically or metaphysically. But even at the physics level, do you see a difference between generating new copies of the world or splitting? [00:50:44] I think it's better to think of in quantum mechanics. In many worlds, the universe splits rather than new copies because people otherwise worry about things like energy conservation. And no one who understands quantum mechanics worries about energy conservation because the equation is perfectly clear. But if all you know is that someone told you the universe duplicates, then you have a reasonable worry about where all the energy for that came from. [00:51:05] So a pre-existing universe splitting into two skinnier universes is a better way of thinking about it. And mathematically, it's just like, you know, if you draw an X and Y axis and you draw a vector of length, one 45 degree angle, you know that you can write that vector of length one as the sum of two vectors pointing along X and Y of length, one over the square root of two. [00:51:28] OK, so I write one arrow as the sum of two arrows, but there's a conservation of Arizona's right now. Two arrows, but the length is the same. [00:51:36] I just am describing it in a different way. And that's exactly what happens when the universe branches the way function of the universe is a big old vector. [00:51:44] So to somebody who brings up a question of saying, doesn't this violate the conservation of energy, can you give a further elaboration? Right. [00:51:56] So let's just be super duper, perfectly clear. [00:51:59] There's zero question about whether or not many worlds violate conservation of energy. Yes, it does not. Great. And I say this definitively because there are other questions that I think there's answers to, but they're legitimate questions. Right, about where this probability comes from and things like that. [00:52:14] This conservation of energy question. We know the answer to it and the answer to it is that energy is conserved. All of the effort goes into how best to translate what the equation unambiguously says into plain English. Right. So this idea that there's a universe that has that the universe comes equipped with the thickness and it sort of divides up into thinner pieces, but the total amount of universe is is conserved over time is a reasonably good way of putting English words to the underlying mathematics. [00:52:44] So one of my favorite things about many worlds is. I mean, I love that there's something controversial in science, and for some reason it makes people actually not like upset, but just get excited. Why do you think it is a controversial idea? So there's there's a lot of it's actually one of the cleanest ways to think about quantum mechanics. So why do you think there's a discomfort a little bit amongst certain people? [00:53:14] Well, I draw the distinction in my book between two different kinds of simplicity in a physical theory. There's simplicity in the theory itself. Right. How we describe what's going on according to the theory, by its own rights. But then, you know, theory is just some sort of abstract mathematical formalism. You have to map it onto the world somehow. Right. And sometimes, like for Newtonian physics, it's pretty obvious, like, OK, here is a bottle and it has a center of mass and things like that. [00:53:43] Sometimes it's a little bit harder with general relativity, curvature of space time is a little bit harder to grasp. [00:53:50] Quantum mechanics is very hard to map. [00:53:53] What you're the language. You're talking in a way functions and things like that onto reality. And many worlds is the version of quantum mechanics where it is hardest to map on the underlying formalism to reality. So that's where the lack of simplicity comes in, not in the theory, but in how we use the theory to map onto reality. And in fact, all of the work in sort of elaborating many worlds, quantum mechanics is in the this effort to map it on to the world that we see. [00:54:21] So it's perfectly legitimate to be bugged by that. Right. To say like, well, no, that's just too far away from my experience. I am therefore intrinsically skeptical of it. Of course, you should give up on that skepticism if there are no alternatives and this theory always keeps working and eventually you should overcome your skepticism. [00:54:40] But right now, there are alternatives that are that, you know, people work to make alternatives that are, by their nature, closer to what we observe directly. Can you describe the alternatives? [00:54:50] I don't think we touched on it. [00:54:52] The Copenhagen interpretation and the many worlds. Maybe there's a difference between the Averett in many worlds and many worlds as it is now, because the idea sort of developed and so on. And just in general, what is the space of promising contenders? We have Democratic debates now. There's a bunch of candidates, 12 candidates, 12 candidates on stage. What are the quantum mechanical candidates on stage for the debate? [00:55:19] So if you had a debate between quantum mechanical contenders, it'd be no problem getting 12 people up there on stage. But there would still be only three frontrunners. [00:55:31] And right now the frontrunners would be Everet. Hidden variable theories are another one. So the hidden variable theory say that the wavefunction is real. But there's something in addition to the wavefunction, the wavefunction is not everything is part of reality, but it's not everything. [00:55:46] What else is there? We're not sure. But the simplest version of the theory, they're literally particles. So many world says that quantum systems are sometimes are wavelike in some ways and particle like in another because they really, really are waves. But under certain observational circumstances they look like particles, whereas hidden variables says they look like waves and particles because there are both waves and particles involved in the dynamics. [00:56:15] And that's easy to do if your particles are just non relativistic Newtonian particles moving around, they get pushed around by the wavefunction roughly. [00:56:24] It becomes much harder when you take quantum field theory or quantum gravity into account. [00:56:30] The other big contenders are spontaneous collapse theories. So in the conventional textbook interpretation, we say when you look at a quantum system, it's wavefunction collapses and you see it in one location. [00:56:43] A spontaneous collapse theory says that every particle has a chance per second of having its way function spontaneously collapse. [00:56:53] The chance is very small for a typical particle that will take hundreds of millions of years before it happens, even once. But in a table or some macroscopic object, there are way more than one hundred million particles and they're all entangled with each other. So when one of them collapses, collapses, it brings everything else along with it. [00:57:10] There's a slight variation of this that the spontaneous collapse theory. There are also induced collapse theories like Roger Penrose thinks that when the gravitational difference between two parts of the wavefunction becomes too large, the wavefunction collapses automatically. So those are basically, in my mind, the three big alternative's many worlds, which is just there's a wavefunction and always a basic Schrodinger equation, hidden variables. There's a wavefunction that always the basis for your equation. [00:57:35] But there are also new variables or collapse theories which the wavefunction sometimes obeys the Schrodinger equation and sometimes it collapses. [00:57:43] So you can see that the alternatives are more complicated in their formalism than. Many worlds is, but they are closer to our experience, so just this moment of collapse, do you think of it as a wavefunction, fundamentally sort of probabilistic description of the world and its collapse, sort of reducing that part of the world into something deterministic, where, again, you can now describe the position and the velocity and the simple classical model? Well, there is how you think about collapse. [00:58:16] There is a fourth category is a fourth contender. There's the mayor of quantum mechanical interpretations, which are called epistemic interpretations. [00:58:25] And what they say is all the wavefunction is, is a way of making predictions for experimental outcomes. It's not mapping onto an element of reality in any real sense. [00:58:36] And in fact, two different people might have two different wave functions for the same physical system because they know different things about it. Right. The way function is really just a prediction mechanism. And then the problem with those epistemic interpretations is if you say, OK, but it's predicting about what? Like what is the thing that is being predicted? [00:58:55] And they say, no, no, no, that's not what we're here for. We're just here to tell you what the observational outcomes are going to be. [00:59:01] But the other the other interpretations kind of think that the way function is real. [00:59:05] Yes, that's right. So that's an authentic interpretation of the wavefunction, ontology being the study of what is real, what exists, as opposed to an epistemic interpretation of the wavefunction epistemology being the study. [00:59:18] What we know that we actually just love to see that debate on stage. [00:59:23] There was a version of it on stage at the World Science Festival a few years ago that you can look up online and YouTube. Yep, it's on YouTube. OK, awesome. I'll take it and watch it. For one year I won. [00:59:36] And of course, I don't know. There was no candidate. There was no vote. But the those there's Bryan Green was the moderator and David Albert stood up for spontaneous collapse. And Shelley Goldstein was there for hidden variables. And Ruediger shock was there for epistemic approaches. [00:59:51] Why do you I think you mentioned it, but just to elaborate, why do you find many worlds so compelling? [00:59:59] Well, there's two reasons, actually. One is, like I said, it is the simplest, right? It's like the most bare bones, austere, pure version of quantum mechanics. And I am someone who is very willing to put a lot of work into mapping the formalism on to reality. I'm less willing to complicate the formalism itself. But the other big reason is that there's something called modern physics with quantum fields and quantum gravity and holography and spacetime doing things like that. [01:00:26] And when you take any of the other versions of quantum theory, they bring along classical baggage, all of the other versions of quantum mechanics. [01:00:36] Prejudice or privilege, some version of classical reality like locations in space. OK, and I think that that's a barrier to doing better at understanding the theory of everything and understanding quantum gravity and the emergence of space time. [01:00:51] Whenever if you change your theory from, you know, here's a harmonic oscillator, oh, there's a spin. Here's an electromagnetic field in hidden variable theories or dynamical collapse theories, you have to start from scratch. You to say like, well, what are the hidden variables for this theory or how does it collapse or whatever, whereas many worlds is plug and play. You tell me the theory and I can give you as many worlds version. So when we have a situation like we have with gravity in spacetime, where the classical description seems to break down in a dramatic way, then I think you should start from the most quantum theory that you have, which is really many worlds. [01:01:24] So start with the quantum theory and try to build up a model of spacetime. The emergence of space time. That's right. OK, so I thought spacetime was fundamental. [01:01:38] Yeah. So this sort of dream that Einstein had, that everybody had and everybody has of, you know, the theory of everything. So how do we build up from many worlds, from quantum mechanics, a model of spacetime, model of gravity? [01:01:56] Well, yeah. I mean, let me first mention very quickly why we think it's necessary, you know? We've had gravity in the form that Einstein bequeathed to us for over a hundred years now, like 1915 and 1916, he put general relativity in the final form. So gravity is the curvature of space time. And there's a field that pervades all the universe that tells us how curved space time is. And that's a fundamentally classical. That's totally classical. [01:02:20] Right, exactly. But we also have a formalism, an algorithm for taking a classical theory and quantifying it. This is how we get quantum electrodynamics, for example. And it could be tricky. I mean, you think you're quantifying something. So that means taking a classical theory and promoting it to a quantum mechanical theory. But you can run into problems. So they ran into problems and they did that with electromagnetism, namely that certain quantities were infinity. And you don't like infinity, right? [01:02:47] So Feynman and Tominaga and Schwager won the Nobel Prize for teaching us how to deal with the infinities. And then Ken Wilson went to another Nobel Prize for saying you shouldn't have been worried about those infinities after all. [01:02:58] But still, that was it's always the thought that that's how you will make a good quantum theory. You'll start with the classical theory and quantize it. So if we have a classical theory, general relativity, we can quantize it or we can try to. [01:03:10] But we run into even bigger problems with gravity than we ran into with electromagnetism. [01:03:15] And so far, those problems are insurmountable. We've not been able to get a successful theory of gravity, quantum gravity, by starting with classical general relativity and quantize it. [01:03:25] And there's evidence that there's a good reason why this is true, that the whatever the quantum theory of gravity is, it's not a field theory. It's something that has weird nonlocal features built into it somehow that we don't understand. And we get this idea from black holes and hawking radiation and information conservation and a whole bunch of other ideas I talk about in the book. So if that's true, if the fundamental theory isn't even local in the sense that an ordinary quantum field theory would be, then we just don't know where to start in terms of getting a classical precursor and quantize it. [01:03:59] So the only sensible thing is at least the next obvious sensible thing to me would be to say, OK, let's just start intrinsically quantum and work backwards, see if we can find a classical limit. [01:04:08] So the idea of locality, the fact that locality is not fundamental to the nature of our existence, sort of, you know, I guess in that sense, modeling everything as a field makes sense to me. [01:04:24] Stuff that's close by Interac stuff that far away doesn't. So what's what's vocality and why is enough fundamental and how is that even possible? [01:04:34] Yeah, I mean, locality is the answer to the question that Isaac Newton was worried about back at the beginning of our conversation. Right. I mean, how can the Earth know what the gravitational field of the sun is? And the answer, as spelled out by Lipless and Bernstein and others, is that there's a field in between and the way a field works. Is that what's happening to the field at this point in space only depends directly on what's happening at points right next to it. [01:04:59] But what's happening at those points depends on what's happening right next to those, right? So you can build up an influence across space through only local interactions. That's what locality means. What happens here is only affected by what's happening right next to it. That's locality. [01:05:14] The idea of locality is built into every field theory, including general relativity. As a classical theory. It seems to break down when we talk about black holes. And, you know, Hawking told us in the 1970s that black holes radiate, they give off, they will eventually evaporate away. They're not completely black. Once we take quantum mechanics into account and we think we don't know for sure. But most of us think that if you make a black hole out of certain stuff, then like Lipgloss Deman taught us you should be able to predict what that black hole will turn into if it's just orbiting the Schrodinger equation. [01:05:49] And if that's true, there are good arguments that can't happen while preserving locality at the same time. It's just that the information seems to be spread out nonlocal in interesting ways and people. [01:06:01] Should you talk about holography with the Leonard Susskind on your Mindscape podcast? Yes, I have a podcast. [01:06:08] I didn't even mention that I'm terrible. No, I'm going to I'm going to ask you questions about that, too. And I've been not shutting up about it's my favorite science podcast or not. It's the same science podcast. It's like it's a scientist doing a part. That's right. That's what it is. Absolutely. Yes. Yeah. Anyway, yeah. [01:06:27] So holography is this idea when you have a black hole and black hole is a region of space inside of which gravity is so strong that you can't escape. And there's this weird feature of black holes that again is totally a thought experiment feature because we haven't gone and probed any yet. But there seems to be one way of thinking about what happens inside a black hole as seen by an observer who's falling in, which is actually pretty normal, like everything looks pretty normal until you hit the singularity and you die. [01:06:54] But from the point of view of the outside observer, it seems like all the information that that fell in. Is actually smeared over the horizon in a nonlocal way, and that's puzzling, and that's so holography, because that's a two dimensional surface that is encapsulating the whole three dimensional thing inside. Right. [01:07:12] Still trying to deal with that. Still trying to figure out how to get there. [01:07:15] But it's an indication that we need to think a little bit more subtly when we quantized gravity to because you can describe everything that's going on in the three dimensional space by looking at the two dimensional projection of it means that locality doesn't is not necessary. [01:07:32] Well, it means that somehow it's only a good approximation. It's not really what's going on, how we're supposed to feel about that. [01:07:40] I just feel liberated. You know, space is just a good approximation. And this was always going to be true once you started quantized and gravity. So we're just beginning now to face up to the dramatic implications of quantize and gravity. [01:07:56] Is there other weird stuff that happens to quantum mechanics and Blackhall? I don't think that anything weird has happened with quantum mechanics, weird things happen with space time. I mean, that's what it is like. Quantum mechanics is still just quantum mechanics, but our ordinary notions of space time don't really quite work. [01:08:14] And there's a principle that goes hand in hand with holography called complementarity, which says that there's no one unique way to describe what's going on inside a black hole. [01:08:28] Different observers will have different descriptions, both of which are accurate but sound completely incompatible with each other. So depends on how you look at it. You know, the word complementarity in this context is borrowed from Niels Bohr, who points out you can measure the position or you can measure the momentum. You can't measure both at the same time in quantum mechanics. [01:08:49] So a couple of questions on many worlds. How does many worlds help us understand our particular branch of reality? OK, that's fine and good. That is, everything is splitting. We're just traveling down a single branch. So how does it help us understand our little unique branch? [01:09:08] Yeah, that's a that's a great question. But that's the point is that we didn't invent many worlds because we thought it was cool to have a whole bunch of worlds. Right. We invented it because we were trying to account for what we observe here in our world and what we observed here in our world, our way functions collapsing. [01:09:23] OK, we do have a position, a situation where the electron seems to be spread out. But then when we look at it, we don't see it spread out. We see it located somewhere. So what's going on? That's the measurement problem of quantum mechanics. That's what we have to face up to so many worlds is just a proposed solution to that problem. And the answer is nothing special is happening. It's still just the Schrodinger equation. But you have a wavefunction, too, and that's a different answer than would be given in hidden variables or dynamical collapse theories or whatever. [01:09:53] So the entire point of many worlds is to explain what we observe, but it tries to explain what we already have observed. Right. It's not trying to be different from what we've observed because that would be something other than quantum mechanics. [01:10:07] But, you know, the idea that there's a world that we didn't observe that keep branching off is kind of is, you know, stimulating to the imagination. [01:10:17] So is it possible to hop? From you mentioned, the branches are independent, yes. Is it possible to hop from one to the other? No, it's the physical limit. The theory says it's impossible is already a copy of you in the other world. [01:10:34] Don't worry. Yes. Leave them alone. [01:10:38] But there's a there's a fear of missing out Fumo. Yes. That I feel like immediately start to wonder if that other copy is having more or less fun. [01:10:50] Well, the downside to many worlds is that you're missing out on an enormous amount and that's always what it's going to be like. [01:10:57] And I mean, there's a certain stage of acceptance in that. Yes. [01:11:01] In terms of rewinding, you think we can rewind the system back? Sort of. [01:11:06] The nice thing about many worlds, I guess, is it really emphasizes the maybe you can correct me, but the determine the deterministic nature of a branch and it feels like it can be wound back. Is it is Dukas is something that can be perfectly run back. [01:11:27] Rewind it back. [01:11:29] Yeah. [01:11:29] You know, if if you had a fancy French restaurant and there's a nice linen white tablecloth and you have your glass of Bordeaux and you knock it over and the wine spills across the tablecloth, if the world were classical, OK, it would be possible that if you just lifted the wine glass up, you'd be lucky enough that every molecule of wine would hop back into the glass. [01:11:50] Right. But guess what? It's not going to happen in the real world. And the quantum function is exactly the same way. It is possible in principle to rewind everything. If you start from perfect knowledge of the entire wavefunction of the universe in practice, it's never going to happen. [01:12:06] So time travel not possible? No. At least quantum mechanics has no help. [01:12:14] What about memory? Does the universe have a memory of itself where we could. In in so not time travel, but peak back in time and do a little like replay. [01:12:31] Well, it's exactly the same in quantum mechanics as classical mechanics. So whatever you want to say about that, you know, the fundamental laws of physics in either many worlds, quantum mechanics or Newtonian physics, conserve information. So if you have all the information about the quantum state of the world right now, you're lipless demon like in your knowledge, calculational capacity. [01:12:53] You can win the clock backward, but none of us is right. And so in practice, you can never do that. You can do experiments over and over again, starting from the same initial conditions for small systems. But once things get to be large, Avogadro's number of particles. [01:13:08] Right, bigger than a cell, no chance. [01:13:12] We we talked a little bit about Arrow of Time last time, but in many worlds that there is a kind of. Implied arrow of time, right? So you've talked about the arrow of time that has to do with the second or third of dynamics. That's the arrow of time. That's emergent or fundamental. We don't know, I guess. [01:13:36] No, it's emergent. It's a is that is everyone agree on that? Well, no, I think they should. [01:13:45] So that area of time is that different than the arrow of time that's implied by many worlds? [01:13:51] It's not different, actually, no. In both cases, you have fundamental laws of physics that are completely reversible. If you give me the state of the universe at one moment in time, I can run the clock forward or backward equally. Well, there's no arrow of time built into the laws of physics that the most fundamental level. [01:14:08] But what we do have are special initial conditions 14 billion years ago near the Big Bang in thermodynamics. Those special initial conditions take the form of things were low. Entropy and entropy has been increasing ever since, making the universe more disorganized and chaotic. And that's the arrow of time in quantum mechanics. The special initial conditions take the form of there was only one branch of the wavefunction and the universe has been branching more and more ever since. [01:14:38] OK, so if time is emergent, so it seems like our human cognitive capacity likes to take things that are emergent and assume and feel like they're fundamental. [01:14:50] So what sort of times? Emergent and locality. Like space emergency? Yes, OK, but I didn't say time was emergency, I said the arrow of time was emergent. Those are different. [01:15:05] What's the difference between the era of time and time? Are you using arrow time to simply mean they're synonymous with the second law of thermodynamics? [01:15:15] No, but the arrow of time is the difference between the past and future. So there's space, but there's no arrow of space. You don't feel that space has to have an arrow, right? You could live in thermodynamic equilibrium. There'd be no arrow of time, but there'd still be time to still be a difference between now and the future or whatever. [01:15:32] OK, so if nothing changes, there's still time. [01:15:36] Well, things could even change. Like if the whole universe consisted of the earth going around the sun. Yeah, OK. It would just go in circles or ellipses. [01:15:45] Right. And things would change. But it's not increasing entropy. There's no arrow. If you took a movie of that and I played you the movie backward, you would never know. So the arrow of time can theoretically point in the other direction for brief, briefly, so important that it points in different directions, it's not a very good arrow. [01:16:06] I mean, the arrow of time in the macroscopic world is so powerful that there's just no chance of going back. [01:16:12] When you get down to tiny systems with only three or four moving parts, then entropy can fluctuate up and down. [01:16:17] What does it mean for space to be an emergent phenomena? [01:16:20] It means that the fundamental description of the world does not include the word space. It will be something like a vector in Hilbert space. Right. And you have to say, well, why is there a good approximate description which involves three dimensional space and stuff inside it? [01:16:35] OK, so time and space are emergent. We kind of mentioned in the beginning. [01:16:40] Can you elaborate? What do you feel? Hope is fundamental in our universe. [01:16:47] A wavefunction living in Hilbert space, wavefunction Hubble space that we can't intellectualize or visualize. [01:16:53] Really, we can't visualize it. [01:16:55] We can intellectualize it very easily, like, well, how do you think about it's a vector in a ten of the ten to one hundred twenty three dimensional vector space, the complex vector unit Naum. [01:17:05] It evolves according to the Schrodinger equation, that when you put it that way, what's so hard really is the quantum computers. [01:17:18] There's some excitement. Actually, a lot of excitement with people that it will allow us to simulate quantum mechanical systems. What kind of questions do about quantum mechanics, about the things we've been talking about? Do you think do you hope we can answer through quantum simulation? [01:17:38] Well, I think that there are there's a whole fascinating frontier of things you can do with quantum computers, both sort of practical things with cryptography or money, privacy, eavesdropping, sorting things, simulating quantum systems. Right. [01:17:57] So it's a broader question, maybe even outside of quantum computers, some of the theories that we've been talking about. What's your hope? What's most promising to test these theories? [01:18:09] What are what are kind of experiments we can conduct, whether in simulation or in the physical world that would validate or disprove or expand these theories? [01:18:20] Well, I think for there's two parts of that question. [01:18:24] One is many worlds and the other one is sort of emergent space time for many worlds. You know, there are experiments ongoing to test whether or not we function spontaneously, collapse. [01:18:34] And if they do, then that rules out many worlds and that would be falsified. [01:18:38] What if there are hidden variables? There's a theorem that seems to indicate that the predictions will always be the same as many worlds. I'm a little skeptical of this theorem. I'm not complete. I haven't internalized that, haven't made it in part of my intuitive view of the world yet. So there might be loopholes to that theorem. I'm not sure about that. Part of me thinks that there should be different experimental predictions if there are hidden variables, but I'm not sure. [01:19:02] But otherwise, it's just quantum mechanics all the way down, and so there's there's this cottage industry in science journalism of writing breathless articles that say, you know, quantum mechanics shown to be more astonishing than ever before thought. [01:19:15] And really it's the same quantum mechanics we've been doing since nineteen twenty six. [01:19:19] Whereas with the emergent spacetime stuff, we know a lot less about what the theory is. It's in a very primitive state. We don't even really have a safely written down, respectable, honest theory yet. [01:19:31] So there could very well be experimental predictions we just don't know about yet. [01:19:34] That is one of the things that we're trying to figure out for emergency spacetime. You need really big stuff, right? [01:19:41] Well, or really fast stuff or really energetic stuff. We don't know. That's the thing, you know. [01:19:46] So there could be violations of the speed of light if you have emergent space time not going faster than the speed of light, but the speed of light could be different for light of different wavelengths. [01:19:58] Right. That'll be a dramatic violation of physics as we know it. But it could be possible or not. I mean, it's not an absolutely prediction. That's the problem. [01:20:07] The theories are just not well developed enough yet to say is there anything that quantum mechanics can teach us about human nature or the human mind? [01:20:18] Do you think about sort of consciousness and these kinds of topics? Isn't it certainly excessively used? As you point out, the word quantum is used for everything besides quantum mechanics. But in more seriousness, is there something? That goes to the human level and can help us understand our mind, not really is the short answer. [01:20:45] You know, minds are pretty classical. I don't think we don't know this for sure, but I don't think that phenomena like entanglement are crucial to how the human mind works or about consciousness. [01:20:57] So you mentioned, I think early on in the conversation, you said it would be a maybe it would be unlikely, but incredible if sort of the observer is somehow a fundamental part of sort of observer not to romanticize the notion, but seems interlinked to the idea of consciousness. So if consciousness is, as the Pensacola's believe is fundamental to the universe, is that possible? Is that wait? [01:21:27] I mean, it is possible, just like you say. Jarobi likes to say it's entirely possible, but. OK, but is it on a spectrum of crazy out there? [01:21:39] How how statistically speaking, how often do you ponder the possibility that consciousness is fundamental or the observer is fundamental to personally don't at all? [01:21:50] There are people who do. I'm a thorough physicalist when it comes to consciousness. I do not think that there are any separate mental states or mental properties. I think they're all emergent, just like spacetime is, and space time is hard enough to understand. So the fact that we don't yet understand consciousness is not at all surprising to you. [01:22:09] As we mentioned. Have an amazing podcast called Mindscape. It's, as I said, one of my favorite podcasts sort of or both for your explanation of physics, which a lot of people love. [01:22:22] And when you venture out into things that are beyond your expertise but is just a really smart person exploring even questions like, you know, morality, for example, was very interesting. [01:22:37] I think it did a solo episode and so on. I mean, there's a lot of really interesting conversations that you have. What are what are some from memory, amazing conversations that pop to mind that you've had. What did you learn from them? Something that may be changed your mind and just inspired you or just this whole experience of having conversations? What stands out to you? It's an unfair question. Totally unfair, but OK, that's all right. [01:23:05] You know, it's often the ones I feel like the ones I do on physics and closely related science or even philosophy ones are like, I know this stuff and I'm helping people learn about it, but I learn more from the ones I have nothing to do with physics or philosophy. Right. So talking to Wynton Marsalis about jazz or talking to a master sommelier about wine, talking to Will Wilkinson about partisan polarization and the urban rural divide, talking to psychologists like Harold Tavaris about cognitive dissonance and how those things work. [01:23:43] Scott Derrickson, who is the director of the movie Dr. Strange, I had a wonderful conversation with him where we went through the mechanics of making a blockbuster superhero movie. Right. And he's also not a naturalist. He's a he's an evangelical Christian. So we talked about the nature of reality there. [01:24:00] I want to have a couple more discussions with. Highly educated theists who know that theology really well, but haven't quite arranged those yet. [01:24:13] I would love to hear that. I mean, that's how comfortable are you venturing into questions of religion? [01:24:20] Oh, I'm totally comfortable doing it. You know, I did talk with Alan Lightman, who is also an atheist, but he he he is trying to rescue the sort of spiritual side of things for atheism. [01:24:33] And I did talk to a very vocal atheist like Alex Rosenberg. So I need to talk to some I've talked to some religious believers, but he talked more. [01:24:43] How have you changed through having all these conversations? You know, part of the motivation was I had a long stack of books that I hadn't read and I couldn't find time to read them, and I figured if I interviewed their authors forced me to read them. [01:24:56] Right. And that's that is totally worked, by the way. Now, I'm annoyed that people write such long books. [01:25:02] I think I'm still very much learning how to be a good interviewer. I think that's a skill that, you know, I think I have good questions. But, you know, there's the the give and take that is still I think I could be better. [01:25:16] Like, I want to offer something to the conversation, but not too much. Right. I've had conversations where I barely talked at all and I had conversations where I talked half the time. I think there's a happy medium in between there. [01:25:26] So I think I remember listening to without mentioning names, some of your conversations where I wish you would have disagreed more. Yeah. As a listener is more fun sometimes. [01:25:38] Well, this is a that's a very good question because, you know, my everyone has an attitude toward that. Like, some people are really there to basically give their point of view. And the their their guest is supposed to, you know, respond accordingly. [01:25:52] I want to sort of get my view on the record, but I don't want to dwell on it when I'm talking to someone like David Chalmers, who I disagree with a lot. You know, I want to say, like, here's why I disagree with you. But, you know, I I'm we're here to listen to you. Like, I have an episode every week, and you're only on once a week. Right. So I have an upcoming podcast episode with Phillip Goff, who is much more dedicated like guest. [01:26:18] And so there we really get into it. [01:26:20] I think that I probably have disagreed with him more on that episode than I ever have with another podcast guest, but that's what he wanted. [01:26:26] So it worked very well. Yeah, yeah. That kind of debate structure is beautiful when it's done right. Like when you're when you can detect that the intent is that you have fundamental respect for the person. Yeah. [01:26:40] That and that's for some reason is super fun to listen to when two really smart people are just arguing and sometimes lose their shit a little bit, if I may say, well, there's a fine line because I have zero interest in bringing I mean, like I mean, maybe you implied this. [01:26:58] I have zero interest in bringing on people for whom I don't have any intellectual respect. Like, I constantly get requests, like, you know, bring on a flat earth or whatever and really slap them down. Recreationists, like I'm a zero interest. [01:27:09] I'm happy to bring on a religious person, a believer, but I want someone who's smart and can act in good faith and can talk, not a charlatan or a lunatic. Right. So I will only I will happily bring on people with whom I disagree, but only people from whom I think the audience can learn something interesting. [01:27:27] So let me ask the idea of Charleton is an interesting idea. [01:27:32] You might be more educated on this topic than me, but there's there's folks, for example, who argue various aspects of evolution, sort of try to approach and say that evolution, sort of our current theory of evolution has many holes in it, as many flaws. [01:27:54] And they argue that I think like Cambridge Cambrian explosion, which is like a huge added variability of species, doesn't make sense under our current description of evolution, the theory of evolution, sort of. [01:28:12] If you were to have the conversation with people like that, how do you know that they're the difference outside the box? Thinkers and people who are fundamentally unscientific and even bordering on charlatans? [01:28:30] It's a great question. And, you know, the further you get away from my expertise, the harder it is for me to really judge exactly those things. And, you know, yeah, I don't have a satisfying answer for that one. [01:28:41] But I think the example you use of someone who, you know, believes in the basic structure of natural selection but thinks that, you know, this particular thing cannot be understood in the terms of our current understanding of Darwinism. That's a perfect edge case where it's hard to tell. Right. And I would have to I would try to talk to people who I do respect and who do know things. [01:29:02] And I would have to, you know, given that I'm a physicist, I know that physicists will sometimes be too dismissive of alternative points of view. I have to take into account that biologists can also be too dismissive of alternative points of view. [01:29:15] So, yeah, that's a tricky one. [01:29:18] Have you gotten heat yet again? He all the time. Like, there's always something. I mean, it's hilarious because I do have I try very hard not to, like, have the same topic several times in a row. I did have like two climate change episodes. They're from very different perspectives, but I like to mix it up. That's the whole point. Well, having fun. And every time I do an episode, someone says, oh, the person you should really get on the talk about exactly that is this other person. [01:29:42] Like, I don't, but I did that. [01:29:43] I want to do that. Well, I hope you keep doing it. You're inspiring millions of people, your books, your podcast. Sean, it's an honor to talk to you. Thank you so much. [01:29:54] Thanks very much.

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