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Entropic Gravity SISSA, Statistical Physics JC Friday 28, 2011 E. Verlinde, arXiv: 1003.4464v2 [hep-th]

Entropic Gravity

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Entropic Gravity. SISSA, Statistical Physics JC Friday 28, 2011. E. Verlinde , arXiv : 1003.4464v2 [ hep-th ]. F. Entropy. Outlook. Background: Holographic Principle (Black Hole Thermodynamics , Entropy Bound ) Verlinde argument for an entropic gravity - PowerPoint PPT Presentation

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Page 1: Entropic Gravity

Entropic Gravity

SISSA, Statistical Physics JCFriday 28, 2011

E. Verlinde, arXiv: 1003.4464v2 [hep-th]

Page 2: Entropic Gravity

F

๐‘ฅ1 ๐‘ฅ2

๐‘ฅ3

๐‘ฅ4

๐‘ฅ5

Entropy

๐‘ฅ5 โ€ฒ

โˆ† ๐‘ฅ ๐‘ญ โˆ†๐‘บ

Page 3: Entropic Gravity

Outlook

โ€ข Background: Holographic Principle (Black Hole Thermodynamics, Entropy Bound)

โ€ข Verlinde argument for an entropic gravity (II principle of dynamics, Newtonโ€™s law of gravity)

โ€ข โ€ฆ editorial discussion

Page 4: Entropic Gravity

Hawking (1971)

Bekenstein (1972)

Hawking (1973)

Black body radiation

๐‘‘๐‘†๐‘š๐‘Ž๐‘ก๐‘ก+๐‘‘๐‘†๐ต๐ปโ‰ฅ0

Page 5: Entropic Gravity

๐‘†๐‘š๐‘Ž๐‘ก๐‘กโ‰ 0 =

๐‘†๐ต๐ป ๐ด

R Bekenstein (1981)

E

A

๐ธ<๐‘€๐ต๐ป

๐‘บ๐’Š๐’=๐‘บ๐’Ž๐’‚๐’•๐’•+๐‘บ๐’”๐’‰๐’†๐’๐’

Susskind (1995)

โ‰ค๐‘บ๐’‡๐’Š๐’=๐‘บ๐‘ฉ๐‘ฏ=๐‘จ๐Ÿ’๐‘€๐ต๐ปโˆ’๐ธ

Page 6: Entropic Gravity

Toward the holographic principleโ€ฆ

๐’…=๐ฅ๐ง๐‘ต=๐’๐’๐’…๐’Š๐’Ž (๐‘ฏ )

Ex 1 ๐‘‘=100 ๐‘™๐‘›2 100 bits of information

Ex 2 !

Number of degrees of freedom

Ex 3 Quantum field theory

๐‘ช๐’†๐’๐’ ๐’”๐’Š๐’›๐’† ๐‘ท๐’๐’‚๐’๐’„๐’Œ ๐‘ณ๐’†๐’๐’ˆ๐’‰๐’• ๐‘Ÿ ๐‘†=๐บ๐‘š๐‘2h ฮฝ=๐‘š๐‘2

๐‘™๐‘=โˆšโ„๐บ๐‘3 =1.6ร—10โˆ’33๐‘๐‘š

๐ธ๐‘›๐‘’๐‘Ÿ๐‘”๐‘ฆ ๐‘ ๐‘๐‘’๐‘๐‘ก๐‘Ÿ๐‘ข๐‘š๐‘๐‘œ๐‘ข๐‘›๐‘‘๐‘’๐‘‘๐‘๐‘ฆ h๐‘ก ๐‘’ ๐‘ƒ๐‘™๐‘Ž๐‘›๐‘๐‘˜๐‘€๐‘Ž๐‘ ๐‘ 

๐‘š๐‘=โˆšโ„๐‘๐บ =1.3ร—1019๐บ๐‘’๐‘‰V oscillators and n states per oscillator

๐‘=๐‘›๐‘‰ ๐‘‘=๐‘‰ ๐‘™๐‘›๐‘›

Page 7: Entropic Gravity

How many different states can be in a region to describe all the physics inside of it?

๐’†๐‘บ ๐’๐’–๐’Ž๐’ƒ๐’†๐’“ ๐’๐’‡ ๐’Ž๐’Š๐’„๐’“๐’๐’”๐’•๐’‚๐’•๐’†๐’”

What is the entropy of the ยซfundamental systemยป?

๐‘†โ‰ค ๐ด4

๐’๐’–๐’Ž๐’ƒ๐’†๐’“ ๐’๐’‡ ๐’ƒ๐’Š๐’•๐’”=๐’…=๐‘จ

๐Ÿ’ ๐‘จ๐‘ท

๐‘=๐‘’๐ด4

A region with boundary of area A is fully described by no more than A/4 degrees of freedom, or about 1 bit of information per Planck area

Page 8: Entropic Gravity

Outlook

โ€ข Background: Holographic Principle (Black Hole Thermodynamics, Entropy Bound)

โ€ข Verlinde argument for an entropic gravity (II principle of dynamics, Newtonโ€™s law of gravity)

โ€ข โ€ฆ editorial discussion

Page 9: Entropic Gravity

SPACE as a storage of information

Holographic screen

โ€ฆ nothing yetโ€ฆ

Emerged space

110011110010001111101001

We further assume the theory has a notion of time and that its dynamics is traslational invariant

EnergyStat. Phys.

Temperature

Page 10: Entropic Gravity

Holographic screen

โˆ† ๐’™

โˆ†๐‘บ=2๐œ‹ ๐‘˜๐‘š๐‘โ„ โˆ† ๐’™ ๐น โˆ†๐‘ฅ=๐‘‡ โˆ†๐‘†

๐’Œ๐‘ป=๐Ÿ๐Ÿ๐…

โ„๐’‚๐’„

โˆ†๐‘บ

๐‘ป

Unruh Effect

๐‘ญ=๐’Ž๐’‚

Force and Inertia

Page 11: Entropic Gravity

Newtonโ€™s law of gravity

๐‘=๐ด๐‘3๐บโ„

๐ธ=12๐‘๐‘˜๐‘‡ ๐ธ=๐‘€๐‘2

โˆ†๐‘บ=2๐œ‹ ๐‘˜๐‘š๐‘โ„ โˆ† ๐’™ ๐น โˆ†๐‘ฅ=๐‘‡ โˆ†๐‘†

Holographic principle

T

๐‘ญ=๐‘ฎ๐‘ด๐’Ž๐‘น๐Ÿ

Page 12: Entropic Gravity

(i) The number of degrees of freedom is proportional to the area of the screen (Holographic principle)

(ii) The energy is evenly distributed over these degrees of freedom

๐‘พ๐’‰๐’‚๐’•๐’‚๐’ƒ๐’๐’–๐’• ๐’•๐’‰๐’†๐’–๐’๐’Š๐’—๐’†๐’“๐’”๐’‚๐’ ๐’„๐’๐’๐’”๐’•๐’‚๐’๐’•๐’” ? ๐’„ ,โ„ ,๐‘ฎ

(iii) There is a change of entropy in the emergent direction

๐‘š๐‘2=12๐‘๐‘˜๐‘‡ Bekenstein + Unruh

โˆ†๐‘บ๐‘ต =๐’Œ ๐’‚โˆ† ๐’™

๐Ÿ๐’„๐Ÿ ๐’‚=โˆ’๐œต๐“ โˆ†๐‘บ๐‘ต =โˆ’๐’Œ โˆ†๐“

๐Ÿ๐’„๐Ÿ

โˆ†๐‘บ=2๐œ‹ ๐‘˜๐‘š๐‘โ„ โˆ† ๐’™ ๐’Œ๐‘ป=๐Ÿ๐Ÿ๐…

โ„๐’‚๐’„

Page 13: Entropic Gravity

ษธ is a coarse-graining variableโˆ†๐‘บ๐‘ต =โˆ’๐’Œ โˆ†๐“

๐Ÿ๐’„๐Ÿ

๐ŸŽ<โˆ’ ๐“๐Ÿ๐’„๐Ÿ<๐Ÿ

Coarse- Graining

Space is emerging!

Amount of coarse graining

Page 14: Entropic Gravity

Dark Energy

radius of the observable universe

holographic principle

๐‘€๐‘2=12 ๐‘๐‘˜๐‘‡=12 ๐ด๐‘˜๐‘‡

๐‘€=1.4 1060๐‘š๐‘Ž๐‘ ๐‘  ๐‘œ๐‘“ h๐‘ก ๐‘’๐‘œ๐‘๐‘ ๐‘’๐‘Ÿ๐‘ฃ๐‘Ž๐‘๐‘™๐‘’๐‘ข๐‘›๐‘–๐‘ฃ๐‘’๐‘Ÿ๐‘ ๐‘’

๐‘˜๐‘‡=๐‘€๐‘2๐ด 10โˆ’ 64

h๐‘ก ๐‘’๐‘’๐‘›๐‘ก๐‘Ÿ๐‘œ๐‘๐‘–๐‘ ๐‘“๐‘œ๐‘Ÿ๐‘๐‘’๐น=๐‘˜๐‘‡ ๐›ป๐‘=๐‘˜๐‘‡๐‘”๐‘Ÿ๐‘Ž๐‘‘ (๐œ‹ ๐‘…2 )=2๐œ‹๐‘˜๐‘‡๐‘…

1๐‘…๐‘‘2๐‘…๐‘‘๐‘ก2

=๐น๐‘€๐‘…=2๐œ‹ ๐‘˜๐‘‡๐‘€ 1.310โˆ’123

Page 15: Entropic Gravity

๐’Œ๐‘ป=๐Ÿ๐Ÿ๐…

โ„๐’‚๐’„Unruh Effect

It works for dimensional consistency!

Page 16: Entropic Gravity

Referencesโ€ข E. Verlinde โ€˜On the origin of Gravity and the Newton

lawsโ€™โ€ข S.Gao Comment on "On the Origin of Gravity and the

Laws of Newton" โ€ข A. Chivukula โ€˜Gravity as an entropic phenomenonโ€™โ€ข T. Jacobson, โ€˜Thermodynamics of Spacetimeโ€™ Phys. Rev.

Lett. (1995)

โ€ข R. Bousso โ€˜The holographic principleโ€™โ€ข R. Ruffini and H. Ohanian โ€˜Gravitation and spacetimeโ€™