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Holography and the Emergence of Gravity Dennis Dieks, Jeroen van Dongen, Sebastian de Haro Reduction and Emergence, MCMP, Munich, 2013

Reduction and Emergence in Holographic Scenarios

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Talk given at the Munich Center for Advanced Studies, conference Reduction and Emergence in the Sciences, Nov. 15, 2013.

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Page 1: Reduction and Emergence in Holographic Scenarios

Holography and the Emergence

of Gravity

Dennis Dieks, Jeroen van Dongen,

Sebastian de Haro

Reduction and Emergence, MCMP,

Munich, 2013

Page 2: Reduction and Emergence in Holographic Scenarios

“Starting from first principles and general assumptions, we present a heuristic argument that shows that Newton’s law of gravitation naturally arises in a theory in which space emerges through a holographic scenario. Gravity is identified with an entropic force caused by changes in the information associated with the position of material bodies.”

Erik Verlinde, 2010

Page 3: Reduction and Emergence in Holographic Scenarios

Philosophical concerns regarding quantum

gravity holography:

• Can one point to a fundamental ontology

with holographically related theories?

• Is one facing emergence of space, time

and/or gravity?

Page 4: Reduction and Emergence in Holographic Scenarios

Overview

• Introduction to holography (Jeroen)

• AdS/CFT and emergence (Sebastian)

• Emergence and Verlinde’s holographic

scenario (Dennis)

Page 5: Reduction and Emergence in Holographic Scenarios

Black hole thermodynamics and

quantum gravity degrees of freedom

• Bekenstein entropy: 𝑆 = 𝐴/4𝐺 (1972)

• Hawking radiation: 𝑇 = 1/8𝜋𝐺𝑀 (1974)

• Information paradox (1985)

• Holographic hypothesis (1993)

• “Maldacena” conjecture: AdS/CFT (1997)

Page 6: Reduction and Emergence in Holographic Scenarios

Holographic hypothesis of ’t Hooft

• The total number of degrees of freedom, 𝑛, in a region of

spacetime containing a black hole is:

𝑛 =𝑆

log 2=

𝐴

4𝐺log 2

• Hence, “we can represent all that happens inside [a volume] by

degrees of freedom on the surface”

• “This suggests that quantum gravity should be described

entirely by a topological quantum field theory, in which all

degrees of freedom can be projected on to the boundary”

Page 7: Reduction and Emergence in Holographic Scenarios

Holographic hypothesis of ’t Hooft

• “We suspect that there simply are no more

degrees of freedom to talk about than the ones

one can draw on a surface [in bit/Planck

length2]. The situation can be compared with a

hologram of a three dimensional image on a

two dimensional surface”

• Fundamental ontology, emergence?

Page 8: Reduction and Emergence in Holographic Scenarios

AdS/CFT

• 𝐷-dim. anti-de Sitter space

• In local coordinates:

d𝑠2 =ℓ2

𝑟2d𝑟2 − d𝑡2 + d𝐱2

• Fields 𝜙 𝑟, 𝑥

• CFT on ℝ𝐷−1

• Operators 𝒪 𝑥

Page 9: Reduction and Emergence in Holographic Scenarios

Duality Statement

• String theory in AdS space = CFT on boundary

• Fields 𝜙 𝑟, 𝑥 ↔ Operators 𝒪 𝑥

• Partition function 𝑑 = 𝐷 − 1 :

𝑍string 𝑟Δ −𝑑𝜙 𝑟, 𝑥 𝑟=0

= 𝜙 0 𝑥 = 𝑒 d𝑑𝑥 𝜙 0 𝑥 𝒪 𝑥

CFT

• One-to-one map of observables.

• Physical equivalence, mathematical structure

different

• Large distance ↔ high energy divergences

Page 10: Reduction and Emergence in Holographic Scenarios

Renormalization Group

• Radial integration: • Wilsonian

renormalization:

Λ 𝑏Λ 0

𝑘

integrate out

New cutoff 𝑏Λ

rescale 𝑏Λ → Λ until 𝑏 → 0

AdS𝑟

𝜕AdS𝑟 𝜕AdS𝜖

new boundary condition

integrate out

IR cutoff 𝜖 in AdS ↔ UV cutoff Λ in QFT

Page 11: Reduction and Emergence in Holographic Scenarios

Philosophical Questions

• Is one side of the duality more

fundamental?

– If QFT more fundamental, space-time could be

‘emergent’

– If duality not exact: room for emergence (e.g.

thermodynamics vs. atomic theory)

• Exact duality: one-to-one relation between

the values of physical quantities

Page 12: Reduction and Emergence in Holographic Scenarios

Remarks

• External view: meaning of observables

externally fixed, map relates different

physical quantities

– No empirical equivalence, numbers correspond

to different physical quantities

• No external point of view:

– How to decide which description to choose?

– Equivalence of descriptions

Page 13: Reduction and Emergence in Holographic Scenarios

• Holography and emergence of gravity?

• Erik Verlinde’s proposal

Page 14: Reduction and Emergence in Holographic Scenarios

Motivating Thoughts

• Hints from string theory, the holographic

conjecture/principle: there are solid indications

from quantum gravity research that gravitational

theories within a volume correspond to a theory

without gravity on the boundary of the volume

• AdS/CFT duality gives a concrete and detailed

example of the idea. Renormalization steps in the

CFT on the surface correspond to different sizes of

the bulk

Page 15: Reduction and Emergence in Holographic Scenarios

Could it be that gravity is “just

the bulk-description” of a world

without gravity?

Page 16: Reduction and Emergence in Holographic Scenarios

Further Motivating Thoughts

• Gravity is special: it is universal. It applies to all

matter and energy, regardless of specific

interactions; it seems to relate to space itself.

• This universality reminds one of the universal

character of thermodynamical behavior, which is

independent of microscopic details

• Gravity distinguishes itself from other forces

because it is difficult to quantize; is it

fundamentally different?

Page 17: Reduction and Emergence in Holographic Scenarios

Program of Research

• Start with a theory without gravity on a two-

dimensional screen, e.g. the surface of a sphere

• Holography: this theory codifies information about

matter in an additional spatial dimension (“in the

bulk”)

• The microscopic details of this gravitation-less

theory remain unspecified: it is a mere information

processing device, a theory of holographic “bits”

• Make gravity appear as a macroscopic

thermodynamic phenomenon

Page 18: Reduction and Emergence in Holographic Scenarios

Guiding idea about force as a

thermodynamic phenomenon

• Entropic processes: as a result of random motion of

its microscopic constituents a physical system will

end up in a state of greater entropy, i.e. higher

probability: the system seems to be directed

• Although there are no forces on the microscopic

level, on the thermodynamic level the system

appears driven, and this can be described by a

“macroscopic force”

• Like an ink droplet in water, or stretched polymer

Page 19: Reduction and Emergence in Holographic Scenarios

Working this out

• Imagine a sphere, whose area is divided into small

cells with each one “bit”. This information suffices

to describe the inside (holography)

• On the sphere an entropic process takes place: the

distribution of 0-s and 1-s tends to an equilibrium

• This process will correspond to gravitational

motion inside the sphere

Page 20: Reduction and Emergence in Holographic Scenarios

Appearance of Space

• In the surface theory, there are no spatial dimensions

other than those within the surface itself

• Consider several spheres, namely different surface

theories that relate to each other via

“renormalization” (or “coarse-graining”)

• “Coarse-grained” theories encode less information,

i.e. describe less space

• Thus, a spatial dimension x appears as a

bookkeeping device that records the level of coarse

graining on the sphere

Page 21: Reduction and Emergence in Holographic Scenarios

The appearance of gravity

• Number of bits on the sphere:

N ~ A = 4πR2

• Equipartition: E = Mc2 ~ N. T

• F = T ∆S/∆x

• ∆S ~ m.∆x

• From which we get: F ~ M.m/R2

Page 22: Reduction and Emergence in Holographic Scenarios

Microscopic theory

on sphere

Microscopic theory

in bulk

Macroscopic theory

in bulk: Gravity

Macroscopic theory

on sphere: no gravity

holography

Thermodynamic

limit

Page 23: Reduction and Emergence in Holographic Scenarios

• The holographic duality relation may well be a

bijective mapping

• There is no reason in this case to think that one side

is more fundamental than the other (left-right)

• But the thermodynamic limit introduces the

emergence of gravity in an uncontroversial sense

(top-bottom)

Page 24: Reduction and Emergence in Holographic Scenarios

Conclusions

• In the holographic scenario, the microscopic surface

theory is not necessarily more fundamental than the

microscopic bulk theory

• However, the appearance of gravity in the

thermodynamic limit makes it a clear case of

emergence, connected with robustness and novelty

of behavior. This robustness explains the

universality of gravitation

• That gravity is emergent could give rise to new

predictions: the law of gravity is not exact but

subject to fluctuations