Brownian Motion in AdS/CFT YITP Kyoto, 24 Dec 2009 Masaki Shigemori (Amsterdam)
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Transcript of Brownian Motion in AdS/CFT YITP Kyoto, 24 Dec 2009 Masaki Shigemori (Amsterdam)
Brownian Motion in AdS/CFTYITP Kyoto, 24 Dec 2009
Masaki Shigemori (Amsterdam)
2
This talk is based on:
J. de Boer, V. Hubeny, M. Rangamani, M.S., βBrownian motion in AdS/CFT,β arXiv:0812.5112.
A. Atmaja, J. de Boer, M.S., in preparation.
3
Introduction / Motivation
4
thermodynamics
Hierarchy of scales in physics
hydrodynamics
atomic theory
subatomic theory
large
small
Scale
macrophysics
microphysics
coarse-grain
Brownian motion
5
AdS BHin classical GR
Hierarchy in AdS/CFT
AdS CFT
[Bhattacharyya+Minwalla+
Rangamani+Hubeny]
thermodynamics of plasma
horizon dynamics
in classical GR
hydrodynamics
Navier-Stokes eq.
quantum BH
strongly coupled quantum plasma
large
small
Scale
long-wavelength approximation
macro-physics
micro-physics
?
This
talk
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Brownian motion
β Historically, a crucial step toward microphysics of nature
1827 Brown
Due to collisions with fluid particles Allowed to determine Avogadro #: NA= 6x1023 < β
Ubiquitous Langevin eq. (friction + random force)
Robert Brown (1773-1858)
erratic motion
pollen particle
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Brownian motion in AdS/CFT
Do the same in AdS/CFT!
Brownian motion of an external quark in CFT plasma
Langevin dynamics from bulk viewpoint?
Fluctuation-dissipation theorem
Read off nature of constituents of strongly coupled plasma
Relation to RHIC physics?Related work:Drag force: Herzog+Karch+Kovtun+Kozcaz+Yaffe, Gubser, Casalderrey-Solana+TeaneyTransverse momentum broadening: Gubser, Casalderrey-Solana+Teaney
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Preview: BM in AdS/CFT
horizon
AdS boundaryat infinity
fundamentalstring
black hole
endpoint =Brownian particle Brownian
motion
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Outline
Intro/motivation
Boundary BM
Bulk BM
Time scales
BM on stretched horizon
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Boundary BM
- Langevin dynamics
Paul Langevin (1872-1946)
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Simplest Langevin eq.
π₯,π= ππ₯αΆ παΆαΊπ‘α»= βπΎ0παΊπ‘α»+ π αΊπ‘α» (instantaneo
us)friction
random force
π αΊπ‘α»Ϋ =Ϋ 0, π αΊπ‘α»π αΊπ‘β²α»Ϋ =Ϋ π 0πΏ(π‘β π‘β²) white noise
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Simplest Langevin eq.
diffusive regime(random walk)
βΰ΅
πππ‘2 (π‘ βͺπ‘πππππ₯)2π·π‘ (π‘ β«π‘πππππ₯)
β’ Diffusion constant:
π·β‘ ππΎ0π
π 2αΊπ‘α»Ϋ β‘Ϋ βαΎπ₯αΊπ‘α»Ϋ π₯αΊ0α»αΏ2 Ϋ
ballistic regime(init. velocity )
π₯αΆ~ΰΆ₯π/π
Displacement:
π‘relax = 1πΎ0 β’ Relaxation time:
(S-E relation) πΎ0 = π 02ππ FD theorem
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Generalized Langevin equation
παΆαΊπ‘α»= βΰΆ± ππ‘β²π‘ββ πΎαΊπ‘β π‘β²α»παΊπ‘β²α»+ π αΊπ‘α»+ πΉ(π‘)
delayed
friction
random force
π αΊπ‘α»Ϋ =Ϋ 0, π αΊπ‘α»π αΊπ‘β²α»Ϋ =Ϋ π (π‘β π‘β²)
external force
Qualitatively similar to simple LE ballistic regime diffusive regime
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Time scales
Relaxation timeπ‘relax β‘ 1πΎ0 , πΎ0 = ΰΆ± ππ‘β0 πΎ(π‘)
π αΊπ‘α»π αΊ0α»Ϋ β½Ϋ πβπ‘/π‘coll time elapsed in a single collision
π‘coll
π‘mfp
Typicallyπ‘relax β«π‘mfp β«π‘coll but not necessarily sofor strongly coupled plasma
R(t)
tπ‘mfp
π‘coll
time between collisions
Collision duration time
Mean-free-path time
How to determine Ξ³, ΞΊ
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1. Forced motion
2. No external force,
παΊπα»= π αΊπα»+ πΉαΊπα»πΎαΎπαΏβ ππ β‘ παΊπα»αΎπ αΊπα»+ πΉαΊπα»αΏ
πΉαΊπ‘α»= πΉ0πβπππ‘
παΊπ‘α»Ϋ =Ϋ παΊπα»πΉ0πβπππ‘
ππΫ =Ϋ a2πa22 π π Ϋ Ϋmeasure
known
read off ΞΌ
read off ΞΊ
admittance
πΉ= 0
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Bulk BM
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Bulk setup
AdSd Schwarzschild BH(planar)
ππ π2 = π2π2 ΰ΅«ββαΊπα»ππ‘2 + ππΤ¦πβ22 ΰ΅―+ π2ππ2π2β(π)
βαΊπα»= 1βαππ»παπβ1
π= 1π½ = αΊπβ 1α»ππ»4ππ2
r
πΤ¦πβ2
horizon
boundary
fundamentalstring
black hole
endpoint =Brownian
particle
Brownian motion
π:AdS radius
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Physics of BM in AdS/CFT
Horizon kicks endpoint on horizon(= Hawking radiation)
Fluctuation propagates toAdS boundary
Endpoint on boundary(= Brownian particle) exhibits BM
transverse fluctuationWhole process is dual to
quark hit by plasma particles
r
πΤ¦πβ2 boundary
black hole
endpoint =Brownian
particle
Brownian motion
kick
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Assumptions
πΤ¦πβ2(π‘,π)
παΊπ‘,πα» r
πΤ¦πβ2
horizon
boundary
Probe approximation
Small gs
No interaction with bulk
Only interaction is at horizon
Small fluctuation
Expand Nambu-Goto actionto quadratic order
Transverse positions aresimilar to Klein-Gordon scalar
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Transverse fluctuations
Quadratic action
π2 = β 14ππΌβ² ΰΆ±ππ‘ ππαπαΆ2βαΊπα»β π4βαΊπα»π4 πβ²2
απ2 + βαΊπα»π4 ππαΊπ4βαΊπα»ππα» ππαΊπα»= 0
παΊπ‘,πα»=ΰΆ± ππβ0 ΰ΅«ππαΊπα»πβπππ‘ππ + h.c.ΰ΅―
d=3: can be solved exactlyd>3: can be solved in low frequency limit
παΊπ‘,πα»
πNG = const + π2 + π4 + β―
Mode expansion
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Bulk-boundary dictionary
Near horizon:
παΊπ‘,πcα»β‘ π₯(π‘) = ΰΆ± ππβ0 οΏ½ππ(ππ)πβπππ‘ππ + h.c.ࡧ
παΊπ‘,πα»βΌΰΆ±ππΞΎ2πβ
0 οΏ½ΰ΅«πβππ(π‘βπβ) + πππππβππ(π‘+πβ)ΰ΅―ππ + h.c.ࡧ outgoin
gmode
ingoingmode
phase shift
πβ
: tortoise coordinate
πc : cutoff
β―π₯αΊπ‘1α»π₯αΊπ‘2α»Ϋ βΫ β ππ1ππ2Ϋ β― Ϋ
observe BMin gauge theory
correlator ofradiation
modesCan learn about quantum gravity in principle!
Near boundary:
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Semiclassical analysis
Semiclassically, NH modes are thermally excited:
AdS3
β ππππΫ βΫ 1ππ½π β 1
Can use dictionary to compute x(t), s2(t) (bulk boundary)
π 2(π‘) β‘ β¨:αΎπ₯αΊπ‘α»β π₯αΊ0α»αΏ2:β© βΫΫ
Ϋ
πππ‘2 (π‘ βͺπ‘relax )πΌβ²ππ2ππ‘ (π‘ β«π‘relax )
π‘relax βΌ πΌβ²ππ2π2
: ballistic: diffusiveDoes exhibit
Brownian motion
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Semiclassical analysis Momentum
distribution
Diffusion constant
Probability distribution for π= ππ₯αΆ παΊπα»β expΰ΅«βπ½πΈπΰ΅―, πΈπ = π22π
Maxwell-Boltzmann
π·= αΊπβ 1α»2πΌβ²8ππ2π
Agrees with drag force computation[Herzog+Karch+Kovtun+Kozcaz+Yaffe]
[Liu+Rajagopal+Wiedemann][Gubser] [Casalderrey-Solana+Teaney]
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Forced motion Want to determine ΞΌ(Ο), ΞΊ(Ο)
β follow the two-step procedure
Turn on electric field E(t)=E0e-iΟt
on βflavor D-braneβ and measure response β¨p(t)β© E(t)p
freely infalling therm
al
b.c. changed from Neumann
βflavor D-braneβ
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Forced motion: results (AdS3) Admittance
Random force correlator
FD theorem
παΊπα»= 1πΎαΎπαΏβ ππ= πΌβ²π½2π2π 1β ππ/ππΌβ²π1β πΌβ²ππ½2π/2π
π αΊπα»= 4ππΌβ²π½3 1βαΊπ½π/2πα»21βαΊπ/2ππΌβ²πα»2 π‘coll βΌ 1π (no Ξ»)
2π Re(πΎαΎπαΏ) = π½π αΊπα» satisfiedcan be proven
generally
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Time scales
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Time scales
R(t)
tπ‘mfp
π‘coll
π‘relax
π‘mfp π‘coll
information about plasma
constituents
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Time scales from R-correlators
R(t) : consists of many pulses randomly distributed
A toy model:
π αΊπ‘α»= πππαΊπ‘β π‘πα»π
π=1 π(π‘) : shape of a single
pulseγγππ = Β±1 : random sign
π : number of pulses per unit time,βΌ 1/π‘mfp
π1 = 1 π2 = 1
π3 = β1
π(π‘β π‘1) π(π‘β π‘2)
βπ(π‘β π‘3) Distribution of pulses = Poisson distribution
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Time scales from R-correlators
Can determine ΞΌ, thus tmfp
π ΰ·¨(π1)π ΰ·¨(π2)Ϋ βΫ 2πππΏ(π1 + π2)πααΊ0α»2
π ΰ·¨αΊπ1α»π ΰ·¨αΊπ2α»π ΰ·¨αΊπ3α»π ΰ·¨αΊπ4α»Ϋ connΫ β 2πππΏ(π1 + π2 + π3 + π4)πααΊ0α»4
tilde = Fourier transform
2-pt func
Low-freq. 4-pt func
π αΊπ‘α»π αΊ0α»Ϋ π‘collβΫ
π ΰ·¨αΊπ1α»π ΰ·¨αΊπ2α»π ΰ·¨αΊπ3α»π ΰ·¨αΊπ4α»Ϋ π‘mfpβΫ
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Sketch of derivation (1/2)
ππαΊπα»= πβππαΊππα»ππ!
Probability that there are k pulses in period [0,Ο]:
π αΊπ‘α»= πππαΊπ‘β π‘πα»π
π=1
π αΊπ‘α»π (π‘β²)Ϋ =Ϋ ππαΊπα»βπ=1 βπππππαΊπ‘Ϋ π‘πα»π(π‘β π‘π) πΫ
ππ,π=1
ππ = Β±1 βΆ random signs β ππππΫ =Ϋ πΏππ
0
k pulses
π‘1 π‘2 π‘π β¦ π
(Poisson dist.)
βπαΊπ‘Ϋ π‘πα»παΊπ‘β² β π‘πα» πΫ = ππΰΆ± ππ’π0 παΊπ‘β π’α»π(π‘β² β π’)
2-pt func:
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Sketch of derivation (2/2)
π αΊπ‘α»π (π‘β²)Ϋ =Ϋ πΰΆ± ππ’βββ παΊπ‘β π’α»π(π‘β² β π’)
π ΰ·¨αΊπα»π ΰ·¨(πβ²)Ϋ =Ϋ 2πππΏαΊπ+ πβ²α»πααΊπα»πα(πβ²)
Similarly, for 4-pt func,
+2πππΏαΊπ+ πβ² + πβ²β² + πβ²β²β² α»πααΊπα»πααΊπβ²α»πααΊπβ²β²α»πααΊπβ²β²β²α» π ΰ·¨αΊπα»π ΰ·¨(πβ²)π ΰ·¨(πβ²β²)π ΰ·¨(πβ²β²β²)Ϋ Ϋπ ΰ·¨αΊπα»π ΰ·¨αΊπβ²α»β© β¨π ΰ·¨(πβ²β²)π ΰ·¨(πβ²β²β²)Ϋ αΊ2 more termsα»+Ϋ
βdisconnected partβ
βconnected
partβ=
π ΰ·¨(π1)π ΰ·¨(π2)Ϋ βΫ 2πππΏ(π1 + π2)πααΊ0α»2
π ΰ·¨αΊπ1α»π ΰ·¨αΊπ2α»π ΰ·¨αΊπ3α»π ΰ·¨αΊπ4α»Ϋ connΫ β 2πππΏ(π1 + π2 + π3 + π4)πααΊ0α»4
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β¨RRRRβ© from bulk BM
Expansion of NG action to higher order: παΊπ‘,πα» πNG = const + π2 + π4 + β―
Can compute tmfp from connected to 4-pt func.
π4 = 116ππΌβ² ΰΆ±ππ‘ ππαπαΆ2βαΊπα»β π4βαΊπα»π4 πβ²22
π π π π Ϋ connΫ Can compute and thus tmfp
4-point vertex
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Holographic renormalization [Skenderis]
Similar to KG scalar, but not quite
Lorentzian AdS/CFT [Skenderis + van Rees]
IR divergence
Near the horizon, bulk integral diverges
β¨RRRRβ© from bulk BM
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Reason: Near the horizon, local
temperature is high String fluctuates wildly Expansion of NG action breaks
down
Remedy: Introduce an IR cut off
where expansion breaks down Expect that this gives
right estimate of the full result
IR divergence
cutoff
35
Times scales from AdS/CFT (weak)
conventional kinetic theory is good
π‘relax ~ πΞΎπ π2 π‘coll ~1π
Resulting timescales:
πβ‘ π4πΌβ²2
weak couplingπβͺ1 π‘relax β«π‘mfp β«π‘coll
π‘mfp ~ 1 πlogΞ»
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Times scales from AdS/CFT (strong)
Multiple collisions occur simultaneously.
strong couplingπβ«1 π‘mfp βͺπ‘coll
Cf. βfast scramblerβ
[Hayden+Preskill] [Sekino+Susskind]
π‘relax ~ πΞΎπ π2 π‘coll ~1π
Resulting timescales:
πβ‘ π4πΌβ²2 π‘mfp ~ 1 πlogΞ»
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BM on stretched horizon
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Membrane paradigm?
Attribute physical properties to βstretched horizonβ
E.g. temperature, resistance, β¦
stretched horizon
actual horizonQ. Bulk BM was due to b.c. at horizon (ingoing: thermal, outgoing: any). Can we reproduce this by interaction between string and βmembraneβ?
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Langevin eq. at stretched horizon
παΊπ‘,πα» r
r=rsr=rH
β#πππαΊπ‘,ππ α»= πΉπ αΊπ‘α» πΉπ (π‘) = βΰΆ± ππ‘β²πΎπ αΊπ‘β π‘β²α»ππ‘παΊπ‘β²,ππ α»+ π π (π‘)π‘
ββ
π π αΊπ‘α»Ϋ =Ϋ 0, π π αΊπ‘α»π π αΊπ‘β²α»Ϋ =Ϋ π π (π‘β π‘β²)
πΉπ αΊπ‘α»
EOM for endpoint: Postulate:
Langevin eq. at stretched horizon
παΊπ‘,π~ππ»α»=ΰΆ±ππΞΎ2π[ππαΊ+α»πβππαΊπ‘βπβα»+ ππαΊβα»πβππαΊπ‘+πβα»+ h.c.]
πΎπ αΊπ‘α»β πΏαΊπ‘α», π π αΊπα»β ΞΎπ ππ(+)
π π αΊπα»β π π αΊπα»Ϋ βΫ ππαΊ+α»β ππαΊ+α»Ϋ βΫ πππ½π β 1
Plug into EOM
Ingoing (thermal)
outgoing (any)
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Friction precisely cancels outgoing
modes
Random force excites ingoing
modes thermally
Can satisfy EOM if
Correlation function:
41
Granular structure on stretched horizon
BH covered by βstringy gasβ[Susskind et al.]
Frictional / random forcescan be due to this gas
Can we use Brownian stringto probe this?
42
Granular structure on stretched horizon AdSd BH
One quasiparticle / string bit per Planck area
Proper distance from actual horizon:
ππ π2 = π2π2 ΰ΅«ββαΊπα»ππ‘2 + ππΤ¦πβ22 ΰ΅―+ π2ππ2π2β(π)
βαΊπα»= 1βαππ»παπβ1
π= 1π½ = αΊπβ 1α»ππ»4ππ2
π₯πβΌ πππ»βπ
π₯π‘ βΌ ΞπΞΎπ βΌ πβπΞΎπ ππ» ππ = αΊ1+ 2πα»ππ» πΏβΌ ΞΎπ π
qpβs are moving at speed of light
(stretched horizon at )
Granular structure on stretched horizon
43
String endpoint collides with a quasiparticle once in time
Cf. Mean-free-path time read off Rs-correlator:
Scattering probability for string endpoint:
Ξπ‘ βΌ βπππΏ
π‘mfp βΌ 1π
π= π₯π‘π‘mfp βΌ βππΏ βΌΰ΅1 (πΏβΌ βP)πs# (πΏβΌ βs)
44
Conclusions
45
Conclusions
Boundary BM β bulk βBrownian stringβ
Can study QG in principle
Semiclassically, can reproduce Langevin dyn. from bulk
random force β Hawking rad. (βkickβ by horizon)
friction β absorption
Time scales in strong coupling QGP: trelax, tcoll, tmfp FD theorem
46
Conclusions
BM on stretched horizon
Analogue of Avogadro # NA= 6x1023 < β?
Boundary:
Bulk:
energy of a Hawking quantum is tiny as compared to BH mass, but finite
πΈ/πβΌ πͺαΊπ2α»< β π/πβΌ πͺαΊπΊπβ1α»< β
47
Thanks!