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Keywords
(9)
adscft correspondence
Degeneration
Gravitational Collapse
Hydrodynamic Limit
Angular Momentum
Black Hole
High Density
Phase Transition
Quark Gluon Plasma
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Degenerate stars and gravitational collapse in AdS/CFT
Degenerate stars and gravitational collapse in AdS/CFT,10.1007/JHEP01(2011)144,Journal of High Energy Physics,Xerxes Arsiwalla,Jan de Boer,Kyriakos Pa
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Degenerate stars and gravitational collapse in AdS/CFT
(
Citations: 6
)
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Xerxes Arsiwalla
,
Jan de Boer
,
Kyriakos Papadodimas
,
Erik Verlinde
We construct composite CFT operators from a large number of fermionic primary fields corresponding to states that are holographically dual to a zero temperature Fermi gas in AdS space. We identify a large N regime in which the fermions behave as free particles. In the
hydrodynamic limit
the Fermi gas forms a degenerate star with a radius determined by the Fermi level, and a mass and
angular momentum
that exactly matches the boundary calculations. Next we consider an interacting regime, and calculate the effect of the gravitational backreaction on the radius and the mass of the star using the TolmanOppenheimerVolkoff equations. Ignoring other interactions, we determine the ”Chandrasekhar limit” beyond which the degenerate star (presumably) undergoes
gravitational collapse
towards a black hole. This is interpreted on the boundary as a
high density
phase transition
from a cold baryonic phase to a hot deconfined phase.
Journal:
Journal of High Energy Physics  J HIGH ENERGY PHYS
, vol. 2011, no. 1, pp. 166, 2011
DOI:
10.1007/JHEP01(2011)144
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Citation Context
(1)
...Similar constructions were considered in [
8
, 9] for neutral and charged free fermion uids supported by a degeneracy pressure...
...It would be interesting to see how the work of [
8
] may be extended for charged uids in order to further characterize the nature of the underlying quantum critical point...
V. Giangreco M. Puletti
,
et al.
Holographic metals at finite temperature
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Citations
(6)
Holographic metals at finite temperature
(
Citations: 2
)
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,
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,
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,
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