From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions ›...

27
From Black holes to Qubits through String Theoretic Microscopes Tadashi Takayanagi Yukawa Institute for Theoretical Physics Kyoto University ICHEP Formal Theory Development, July 10 th , 2018 @ Seoul

Transcript of From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions ›...

Page 1: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

From Black holes to Qubits through String Theoretic Microscopes

Tadashi Takayanagi

Yukawa Institute for Theoretical PhysicsKyoto University

ICHEP Formal Theory Development, July 10th, 2018 @ Seoul

Page 2: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

① Introduction

In biology, chemistry, condensed matter physics etc., various microscopes are crucial experimental devises.

In particle/nuclear physics,accelerators play important roles of microscopes.

What are useful microscopes in string theory, as a promising candidate of quantum gravity ?

Page 3: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

What is string theory ?

Open Strings

Closed Strings

+-

Gravitons,…(Supergravity)

Gauge Fields,Quarks,Leptons,..

However, please do not ask me questions like: How to derive Standard Model from string theory ?Why do we live in 4 dimensions ?How to realize de-Sitter spacetimes in a well-reliable way ?

:String theory is still too infant to give complete answers to them.

Page 4: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Recent studies clearly suggest

Microscopes in string theory = Holographye.g. AdS/CFT (gauge/gravity duality)

Holography is not real experiments but provides a lot of useful thought experiments !

Historically, the most important hint of holographywas the Bekenstein-Hawking Formula 1972-75

of black hole entropy.

Page 5: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

This formula is still mysterious even today. ⇒ looks like “OOPARTS’’

Why entropy in classical theories ?What is quantum Hilbert space of gravity ?

This formula stimulated the recently active subject of emergent spacetime from quantum entanglement.

“It from Qubit’’

(includes too advanced knowledge to digest for a short period)

Ryu-TakayanagiHEE Conjecture 2006

Lewkowycz-MaldacenaProof of HEE

2013Almheiri-Marolf-Polchinski-Sully, Fire wall paradox 2012

Page 6: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Contents① Introduction

② Blackholes and String Theory

③ Aspects of Holography

④ Emergent Spacetime from Quantum Entanglement

⑤ Conclusions

Page 7: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

② Black holes and String Theory

(2-1) Black hole Entropy

Nowadays, black holes (BHs)are getting more familiar astrophyical objects.

e.g. Gravitational waves froma merger of a pair of BHsGW150914 (LIGO,Virgo)

:

Page 8: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

A BH can be produced after a gravitational collapse of a heavy star.

The amount of this hidden information in BHs is measured by the black hole entropy.

BHStar

A lot of informationis hidden in BHs !

×Observer

Page 9: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Bekentein-Hawking Formula of BH Entropy

A= Surface Area of Black hole ⇒Geometry

GN=Newton constant ⇒Gravity

ℏ=Planck constant ⇒Quantum Mechanics

Steven Hawking1942-2018

Jacob Bekenstein1947-2015

BH Entropy is proportional to the area, not to the volume !

Page 10: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Gravity

Gravity on M = Quantum Matter on ∂M

=

Matter

(2-2) HolographyThis suggests

Degrees of Freedom in Gravity ∝ Area .The idea of holographic principle !

[’t Hooft 1993, Susskind 1994]

HolographyBdy of M

Page 11: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

(2-3) Black hole Entropy from String Theory

We need heavy objects to create a black hole.⇒ In string theory, D-branes are very good

examples.

D-branes

Open Strings

Coherent State of Strings

Joseph Polchinski1954-2018

Page 12: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

(ext.) Black holes = D-branes+Open Strings

[Strominger, Vafa 1996]

Dbranes

OpenStrings

??

=

Hawking Radiations

Observer

Holographyas a String Theory Microscope

𝑆𝑆𝐵𝐵𝐵𝐵 =𝐴𝐴

4𝐺𝐺𝑁𝑁

𝑆𝑆𝑆𝑆𝑆𝑆𝑆𝑆𝑆𝑆𝑆𝑆𝑆𝑆 = 2𝜋𝜋 𝑄𝑄1𝑄𝑄5𝑁𝑁

Agree !

BH

Page 13: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Basic Principle (Bulk-Boundary relation):

AdS/CFT

Classical limitLarge N + Strong coupling

CFTGravity ZZ =

Gravity (String theory) on D+1 dim. AdS

(anti de-Sitter space)

Conformal Field Theory (CFT) on D dim.Minkowskispacetime

General relativity with Λ<0

Strongly interacting Quantum Field Theories

③ Aspects of Holography

(3-1) AdS/CFT Correspondence [Maldacena 1997]

=

Page 14: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

N D-branes

Open Strings

EquivalentThermodynamics of various materials

Gravity in Anti de-Sitter space

Thermodynamics ofBlack holes (branes)

EquivalentAdS/CFT

Conformal Field Theories(CFTs)

SU(N) gauge theories

21

22222

zdxdtdz

Rdsd

i i∑=+−

⋅=

Closed Strings

Page 15: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Closed String

Open String

AdS/CFT origins from the open/closed duality:

There is no complete proof of AdS/CFT.

However, we already have O(104) evidencesfor these 20 years.

Page 16: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Strongly Coupled SU(N) gauge Classicaltheories in the large N limit Gravity

Closely related examples:Quark-Gluon plasma

Cold atoms, High Tc SC, etc.

Caution

[Lacey et.al. 2006] [Kovtun-Son-Starinets 2004]

Viscosity/Entropy Ratio

𝜼𝜼𝒔𝒔

=𝟏𝟏𝟒𝟒𝝅𝝅

Closed to the AdS/CFT result

Page 17: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Recent Applications to strongly coupled systems

(1) Quantum Chaos (Lyapunov exponent: λ)

(2) Specific Heat

2D strongly interacting metal (∃Fermi Surface)

λ𝑨𝑨𝑨𝑨𝑨𝑨 =𝟐𝟐π𝒌𝒌𝑩𝑩𝑻𝑻ℏ

λ≤ 𝟐𝟐π𝒌𝒌𝑩𝑩𝑻𝑻ℏIn general, we have .

[Maldacena-Shenker-Stanford 2015]

CAdS∝Tα with (Non Fermi Liquids)cf. α=1 for Landau

Fermi liquids

α≤ 𝟐𝟐𝟑𝟑

[Ogawa-Ugajin-Takayanagi 2011]

[𝑾𝑾 𝒕𝒕 ,𝑽𝑽(𝟎𝟎)]𝟐𝟐 ≈𝟏𝟏𝑵𝑵𝟐𝟐 𝒆𝒆

λ𝒕𝒕

Page 18: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

④ Emergent Spacetime from Quantum Entanglement

(4-1) Quantum Entanglement (QE)

QE = quantum correlations between two subsystems

Simple example: 2 Qubits system

(1) Direct Product StateNot

Entangled(2) EPR (Bell) States

Entangled

BAc ↓⊗↑=ΨA B

( )BABA

↑⊗↓±↓⊗↑=Ψ2

1A B

Page 19: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Entanglement Entropy

Amount of QE =# of EPR Pairs

First we decompose the Hilbert space:

We introduce the reduced density matrix by tracing out B

The entanglement entropy (EE) is defined by

. BAtot HHH ⊗=A BExample:Spin-chain

AS

EntanglementEntropy (EE)

]logTr[ AAAS ρρ−=

Page 20: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

(4-2) Holographic Entanglement Entropy (HEE)[Ryu-Takayanagi 2006]

A

BGravity

(AdS)=

EE in CFT: SA can be computed from the minimal area surface ΓA:

CFT on boundary

Entanglement Wedge

𝑨𝑨𝑨𝑨 = 𝐦𝐦𝐦𝐦𝐦𝐦𝐀𝐀𝐀𝐀𝐀𝐀𝐀𝐀(Γ𝑨𝑨)𝟒𝟒𝑮𝑮𝑵𝑵Γ𝑨𝑨

𝚪𝚪𝐀𝐀Note: The bdy of ΓA =The bdy of A.

Many evidences of this conjecture have been found for these 10 years.

This formula was proved by Lewkowycz-Maldacena 2013 based on the bulk-bdy relation of AdS/CFT.

Page 21: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Recent Updates

(1) Entanglement Wedge

(2) Holographic Entanglement of Purification

NG4)Area()(E AB

ABpΣ

=ρ MAB

ΣAB

A B

Minimal Cross SectionOf Entanglement Wedge

[Umemoto-Takayanagi 2017, Swingle et.al. 2017]

gravity AdSin CFTin

MA

A

ρρ⇔

AΓA

MA

Entanglement Wedge

AdS

[Jafferis-Lewkowycz-Maldacena-Suh 2015, Dong-Harlow-Wall 2016]

Page 22: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Einstein Equation from Quantum Entanglement First Law of EE

[HA=-logρA: Modular Hamiltonian]AA HS ∆≅∆

[Raamsdonk et.al. 2013, Faulkner et.al 2013, 2017, Sarosi-Ugajin. 2017]

[Casini-Huerta-Myers 2013, Bhattachrrya-Nozaki-Ugajin-Takayanagi 2013 ]

AO∂ −∂ −∂ − 2 ∆SA(t, x,l) = Olxll

3

22

Matter contributionsC.C.Kinetic term

φ↔O

The 1st law of EE explains the perturbative Einstein eq.

l

(t,x)

Page 23: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

The HEE suggests that there is one qubit of entanglement for each Planck length area !

B

A

Planck length

As we can change the position and size of A, gravitational spacetimes may consist of EPR pairs !

(4-3) Emergent Spacetime from Qubits

𝑨𝑨𝑨𝑨 =𝐀𝐀𝐀𝐀𝐀𝐀𝐀𝐀(Γ𝑨𝑨)𝟒𝟒𝒍𝒍𝒑𝒑𝒍𝒍𝑫𝑫−𝟏𝟏

∼1065 qubits per 1cm2 !

Page 24: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Tensor Network (TN) and AdS/CFT

Tensor network = Graphical description of quantum states

MERA(Multi-scale Entanglement Renormalization Ansatz)

⇒ a TN suitable for CFTs.

Conjecture [Swingle 2009,…]: a Time slice of AdS= a TN (MERA,..etc.)

⇒MERA(Multi-scale Entanglement Renormalization Ansatz)

[Vidal 2005 ]

Coarse-Graining(Isometry)

MERA TN

AdSMERA TN

Disentangler(Unitary)UV

IRΓAΓA ≈

Page 25: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Dynamics in cMERA [Mollabashi-Nozaki-Ryu-Takayanagi 12,13]

Entanglement dynamics in TN = Gravity Dynamics !

ER=EPR conjecture

Time

Bdy of AdS

Density of QE

AdS horizon Length scale z

[Maldacena-Susskind 2013]

QE between A and B = Wormhole between A and B

This is naturally realized in the AdS/TN conjecture.

Add interactions between A and B make the wormhole traversable (~Quantum Teleportation). [Gao-Jafferis-Wall 2016]

Einstein-Rosen Bridge

Similar to propagation Of Gravitational waves

Page 26: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

⑤ Conclusions• Many efforts to understand the Bekenstein-Hawking

formula has lead to the idea of holography, which plays the central role in string theory currently.

• The AdS/CFT provides a very powerful tool to study quantum gravity or even its definition.

• Studies of quantum entanglement in AdS/CFT inspires the new idea of emergent spacetime from quantum entanglement. Tensor networks is one possibility of a concrete realization of this idea.

Area of minimal surface = Entanglement Entropy Volume of maximal time slice = Complexity

?[Susskind 2014, Adam et.al. 2015]

Page 27: From Black holes to Qubits through String Theoretic ... › event › 686555 › contributions › ... · quantum gravity or even its definition. • Studies of quantum entanglement

Future problems

• An explicit proof of AdS/CFT

• Generalization of AdS/CFT to other spacetimes(e.g. cosmological spacetimes such as de Sitter spaces)

• Clear explanation of Black hole information paradox: show explicitly recovery of information from radiations.

• More quantum information quantities from AdS/CFT (e.g. complexity, mixed state entanglement)

• Holography for open string theory::