Roberto Emparan

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BHs as fluid droplets/lumps Possible fixes: Caldarelli+Dias+RE+Klemm Miyamoto+Maeda • Consider not vacuum bhs, but bhs in AdS – Can tell large and small bhs – Large black holes can fit long-wavelength fluctuations • Small parameter 1/N (number of dimensions): large N expansion – large-N bhs are large
BHs as fluid drops/lumps • Large BHs in AdS: fluid lumps • BHs in gravitational duals to confining theories: AdS with “infrared bottom” • BH is dual to plasma ball: with surface boundary Aharony+Minwalla+Wiseman • “Analogy” upgraded to precise “duality” – although, actually, no independent construction of gravitational side – fluid “prediction” for GL instab of black branes
Page 1 and 2: Black Holes, Fluids, and their Inst
Page 3 and 4: “Black Holes are like Fluids” W
Page 9 and 10: Gregory-Laflamme instability λ=2π
Page 11 and 12: General Relativity as Fluid dyn •
Page 13 and 14: Membrane paradigm • Fluid stress-
Page 15 and 16: BHs as fluid droplets/lumps • Ana
Page 17 and 18: BHs as fluid droplets/lumps • Ray
Page 19: BHs as fluid droplets/lumps • Hig
Page 23 and 24: Fluid/gravity correspondence(s) •
Page 25 and 26: General Classical Brane Dynamics
Page 27 and 28: Blackfold effective theory ∇ µ T
Page 29 and 30: Gregory-Laflamme as sound-mode inst
Page 31 and 32: Viscous damping of sound • Viscos
Page 33 and 34: Gregory-Laflamme as sound-mode inst
Page 35 and 36: Gregory-Laflamme from fluid dynamic
Page 41 and 42: Conclusions • Several meanings to

Roberto Emparan

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