Gravitational collapse and thermalization in the hard wall model

Anastasios Taliotis; Ben Craps; Christopher Rosen; Elias Kiritsis; Hongbao Zhang; Joris Vanhoof

Gravitational collapse and thermalization in the hard wall model

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arxiv 1311.7560 v2 pith:KU2BCOZG submitted 2013-11-29 hep-th

Ben Craps , Elias Kiritsis , Christopher Rosen , Anastasios Taliotis , Joris Vanhoof , Hongbao Zhang This is my paper

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keywords injectionenergyhardholographicmodelsufficientlythermalizationwall

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We study a simple example of holographic thermalization in a confining field theory: the homogeneous injection of energy in the hard wall model. Working in an amplitude expansion, we find black brane formation for sufficiently fast energy injection and a scattering wave solution for sufficiently slow injection. We comment on our expectations for more sophisticated holographic QCD models.

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Dynamics of chiral phase transition in a $N_f=2+1$ soft-wall AdS/QCD model
hep-ph 2025-07 conditional novelty 4.0 of 10

In a 2+1 flavor soft-wall AdS/QCD model, the chiral condensate exhibits slow, non-trivial relaxation with a metastable plateau or overshoot when quenched close to the phase transition.

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