entropy bounds, holography & 2 nd law ( in cosmology )
DESCRIPTION
Ram Brustein. אוניברסיטת בן-גוריון. Entropy Bounds, Holography & 2 nd Law ( in Cosmology ). gr-qc/9904061=PRL 84 (00) hep-th/9907032=PLB 471 (00) with S. Foffa & R. Sturani hep-th/9912055=PRL 8? (00) with G. Veneziano. Entropy bounds, holography, Causal Entropy Bound (CEB) - PowerPoint PPT PresentationTRANSCRIPT
Entropy Bounds, Holography & 2nd Law ( in Cosmology )
אוניברסיטת בן-גוריון
Ram Brustein
Entropy bounds, holography, Causal Entropy Bound (CEB)
Quantum & Geometric entropies
GSL
•gr-qc/9904061=PRL 84 (00)•hep-th/9907032=PLB 471 (00)with S. Foffa & R. Sturani•hep-th/9912055=PRL 8? (00)with G. Veneziano
S,E
ERS
R
BEB :Bekenstein ‘81
Too much entropy/ too little energy ==> GSL
(For systems of limited gravity R>Rg =2 E GN )
Apply BEB to the universe ?! U is not a system of limited gravity …
Bekenstein ‘89
3422
31
,,
,
NTsNTHM
REHR
P
N
M
M
TNH
N
MT
P
P
P
2
4
43
NT
MNTNTRs P
Upper bound on curvature
2
22,
Pl
R
NG
R
NG
RSEERS
2
2
3
3
3PP l
R
l
R
l
V
UV
S
BEB is not compatible with QFT!
QFT:
Holographic principle:Any physical system can be completely specified by data stored on its boundary, without exceeding a density of one bit per Planck area.(adapted from Bousso hep-th/9911002 )
‘tHooft ‘93Susskind ‘95
Holographic entropy bound
2Pl
AHOL
SS But what is S ?
Bousso: use light-sheets=2+1D collections of light-rays orthogonal to surfaceFS: past ingoing light-sheet- wrong!B: 1. light-sheet of decreasing area = “inside” with converging geodesics 2. Stop when caustic ~ singularityneed “space-like projection”
TgTTgxd
RgRRgxdS
P
P
l
lCEB
21
0
41
21
0
41
Max
Max2
0
CEBSS 0CEB :
EVSVE
VS
R.B. & Veneziano ‘00
TgTTs
Pl 211 Max
ppsPl
,Max 31
Local form of CEB :
pppdiagT ,,, in cosmology:
CEB A bound on curvature(for RD FRW)
43 NTMNT PM
NPTH ,
Derivation of CEB :
( i ) Entropy is maximized by the largest stable BH (s) that can fit in a region
( i i) The largest stable BH is determined by causality: BH horizon < RCC
R3CC
R3CC
R3CC
V22
2
3
2
2
3,
PP
HH
P
HH
CC
CC
CC
CC
CC
R
VR
R
VSnS
RS
R
Vn
Find RCC : use cosmological perturbations
BEBCEBHOL
HOLCEBBEB
SSS
SSS
Comparison between entropy bounds
HOLBEBP
CEB SSRER
EVSP
2
211
Bousso is o.k.
limited gravity 2P
ER
not limited gravity 2P
ER
Quantum entropy: Entropy of quantum fluctuations
Modes “freeze”/ “thaw” “exit” / “reenter”
02 2 kkk kH
max
min )(
ln3
k
k kfknkdsquantum
Hquantum nS
NQuantum entropy is real !So what about 2nd law ?
PMk maxConstant !
R3CC
R3CC
R3CC
V
Causal boundaryhas geometric entropy
Proposed resolution: R.B., PRL 84 ‘00
Proof in progress
NG
RH CCGS
2
Entropy bounds: Geometric entropy dominates
0
HH
HH
H
QuantumClassical
NdndSnSdn
dSdSdS
02)()33( HHH
HHHH
H SnNSnH
N
MH P
Generalized second law
In cosmology: 2
2
31
31 ,
)(,
P
HHCC l
HS
H
anHR
2,0 HHH
R.B., PRL 84 ‘00
Conclusions
Holography modified by causality א
Singularity thms. modified by entropy בbounds
Hint: shortest length scale N ג
M P