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Entropic Gravity
SISSA, Statistical Physics JC
Friday 28, 2011
E. Verlinde, arXiv: 1003.4464v2 [hep-th]
F
๐‘ฅ3
๐‘ฅ1
๐‘ฅ2
๐‘ฅ5
๐‘ฅ4
E
n
t
r
o
p
y
๐น=
โˆ†๐‘ฅ
๐œ•๐‘†
๐‘‡
๐œ•๐‘ฅ
๐‘ญ~โˆ†๐‘บ
๐‘ฅ5 โ€ฒ
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
๐’…๐‘จ โ‰ฅ ๐ŸŽ Hawking (1971)
๐‘บ๐‘ฉ๐‘ฏ =
๐‘จ
๐Ÿ’
๐‘‘๐‘†๐‘š๐‘Ž๐‘ก๐‘ก + ๐‘‘๐‘†๐ต๐ป โ‰ฅ 0
Bekenstein (1972)
Black body radiation
๐‘ป=
โ„๐’„๐Ÿ‘
๐Ÿ–๐‘ฎ๐‘ด๐’Œ
Hawking (1973)
๐‘†๐‘š๐‘Ž๐‘ก๐‘ก โ‰  0
๐‘†๐‘š๐‘Ž๐‘ก๐‘ก = 0
๐‘†๐ต๐ป ~๐ด
R
๐‘บ๐’Ž๐’‚๐’•๐’• < ๐Ÿ๐…๐‘ฌ๐‘น Bekenstein (1981)
E
๐ธ < ๐‘€๐ต๐ป
๐‘€๐ต๐ป โˆ’ ๐ธ
๐‘บ๐’Š๐’
= ๐‘บ๐’Ž๐’‚๐’•๐’• + ๐‘บ๐’”๐’‰๐’†๐’๐’ โ‰ค
A
๐‘บ๐’Ž๐’‚๐’•๐’• โ‰ค
๐‘จ
๐Ÿ’
๐‘บ๐’‡๐’Š๐’
= ๐‘บ๐‘ฉ๐‘ฏ
๐‘จ
=
๐Ÿ’
Susskind (1995)
Toward the holographic principleโ€ฆ
๐’… = ๐ฅ๐ง ๐‘ต = ๐’๐’ ๐’…๐’Š๐’Ž(๐‘ฏ)
Ex 1 ๐Ÿ๐ŸŽ๐ŸŽ ๐’”๐’‘๐’Š๐’ ๐‘ = 2100 ๐‘ ๐‘ก๐‘Ž๐‘ก๐‘’๐‘ 
Ex 2
๐‘ฏ๐’‚๐’“๐’Ž๐’๐’๐’Š๐’„ ๐’๐’”๐’„๐’Š๐’๐’๐’‚๐’•๐’๐’“
Ex 3
Quantum field theory
Number of degrees of freedom
๐‘‘ = 100 ๐‘™๐‘›2
๐‘ช๐’†๐’๐’ ๐’”๐’Š๐’›๐’† ~๐‘ท๐’๐’‚๐’๐’„๐’Œ ๐‘ณ๐’†๐’๐’ˆ๐’‰๐’•
100 bits of information
๐‘ = โˆž!
โ„Žฮฝ = ๐‘š๐‘ 2
๐‘™๐‘ =
๐บ๐‘š
๐‘Ÿ๐‘† = 2
๐‘
โ„๐บ
= 1.6 × 10โˆ’33 ๐‘๐‘š
3
๐‘
๐ธ๐‘›๐‘’๐‘Ÿ๐‘”๐‘ฆ ๐‘ ๐‘๐‘’๐‘๐‘ก๐‘Ÿ๐‘ข๐‘š ๐‘๐‘œ๐‘ข๐‘›๐‘‘๐‘’๐‘‘ ๐‘๐‘ฆ ๐‘กโ„Ž๐‘’ ๐‘ƒ๐‘™๐‘Ž๐‘›๐‘๐‘˜ ๐‘€๐‘Ž๐‘ ๐‘ 
V oscillators and n states per oscillator
๐‘ = ๐‘›๐‘‰
๐‘‘ = ๐‘‰ ๐‘™๐‘› ๐‘›
๐‘š๐‘ =
โ„๐‘
= 1.3 × 1019 ๐บ๐‘’๐‘‰
๐บ
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 «fundamental system»?
๐ด
๐‘†โ‰ค
4
๐‘=
๐ด
๐‘’4
๐‘จ
๐’๐’–๐’Ž๐’ƒ๐’†๐’“ ๐’๐’‡ ๐’ƒ๐’Š๐’•๐’” = ๐’… =
๐Ÿ’๐‘จ๐‘ท
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
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
SPACE as a storage of information
โ€ฆ nothing yetโ€ฆ
110
011
110
010
001
111
101
001
Emerged space
Holographic screen
We further assume the theory has a notion of time and that its dynamics is traslational invariant
Energy
Temperature
Stat. Phys.
Force and Inertia
โˆ†๐‘บ
๐‘ป
โˆ†๐’™
Holographic screen
๐‘š๐‘
โˆ†๐‘บ = 2๐œ‹๐‘˜
โˆ†๐’™
โ„
๐’Œ๐‘ป =
๐นโˆ†๐‘ฅ = ๐‘‡โˆ†๐‘†
๐Ÿ โ„๐’‚
๐Ÿ๐… ๐’„
Unruh Effect
๐‘ญ = ๐’Ž๐’‚
Newtonโ€™s law of gravity
Holographic principle
๐ด๐‘ 3
๐‘=
๐บโ„
๐‘š๐‘
โˆ†๐‘บ = 2๐œ‹๐‘˜
โˆ†๐’™
โ„
๐ธ=
1
๐‘๐‘˜๐‘‡
2
๐ธ = ๐‘€๐‘ 2
๐นโˆ†๐‘ฅ = ๐‘‡โˆ†๐‘†
๐‘ฎ๐‘ด๐’Ž
๐‘ญ=
๐‘น๐Ÿ
T
(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
1
= ๐‘๐‘˜๐‘‡
2
Bekenstein + Unruh
โˆ†๐‘บ = 2๐œ‹๐‘˜
โˆ†๐‘บ
๐’‚โˆ†๐’™
=๐’Œ ๐Ÿ
๐‘ต
๐Ÿ๐’„
๐’‚ = โˆ’๐œต๐“
๐‘š๐‘
โˆ†๐’™
โ„
๐’Œ๐‘ป =
๐Ÿ โ„๐’‚
๐Ÿ๐… ๐’„
โˆ†๐‘บ
โˆ†๐“
= โˆ’๐’Œ ๐Ÿ
๐‘ต
๐Ÿ๐’„
ษธ is a coarse-graining variable
โˆ†๐‘บ
โˆ†๐“
= โˆ’๐’Œ ๐Ÿ
๐‘ต
๐Ÿ๐’„
๐“
๐ŸŽ<โˆ’ ๐Ÿ<๐Ÿ
๐Ÿ๐’„
Amount of coarse graining
Coarse- Graining
Space is emerging!
Dark Energy
๐‘…~2.7 1061 radius of the observable universe
๐‘ = ๐ด = ๐œ‹๐‘…2 holographic principle
1
1
๐‘€๐‘ 2 = ๐‘๐‘˜๐‘‡ = ๐ด๐‘˜๐‘‡
2
2
๐‘€ = 1.4 1060 ๐‘š๐‘Ž๐‘ ๐‘  ๐‘œ๐‘“ ๐‘กโ„Ž๐‘’ ๐‘œ๐‘๐‘ ๐‘’๐‘Ÿ๐‘ฃ๐‘Ž๐‘๐‘™๐‘’ ๐‘ข๐‘›๐‘–๐‘ฃ๐‘’๐‘Ÿ๐‘ ๐‘’
๐‘€๐‘ 2
๐‘˜๐‘‡ =
~10โˆ’64
๐ด
๐‘กโ„Ž๐‘’ 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‘…
1 ๐‘‘2 ๐‘…
๐น
๐‘˜๐‘‡
โˆ’123
=
=
2๐œ‹
~1.3
10
๐‘… ๐‘‘๐‘ก 2 ๐‘€๐‘…
๐‘€
Unruh Effect
๐Ÿ โ„๐’‚
๐’Œ๐‘ป =
๐Ÿ๐… ๐’„
It works for dimensional consistency!
References
โ€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€™