Gravitational collapse and thermalization in the hard wall model - INSPIRE

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Gravitational collapse and thermalization in the hard wall model

Ben Craps
(
- Vrije U., Brussels and
- Intl. Solvay Inst., Brussels
)
,
Elias Kiritsis
(
- APC, Paris and
- CERN and
- Crete U.
)
,
Christopher Rosen
(
- Crete U.
)
,
Anastasios Taliotis
(
- Vrije U., Brussels and
- Intl. Solvay Inst., Brussels
)
,
Joris Vanhoof
(
- Vrije U., Brussels and
- Intl. Solvay Inst., Brussels
)

Nov 29, 2013

28 pages

Published in:

JHEP 02 (2014) 120

Published: 2014

e-Print:

1311.7560 [hep-th]

DOI:

10.1007/JHEP02(2014)120

Report number:

CERN-PH-TH-2013-267

View in:

reference search42 citations

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Abstract: (arXiv)

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.

Note:

33 pages, 5 figures

Holography and quark-gluon plasmas
Gauge-gravity correspondence
energy: injection
quantum chromodynamics: holography
field theory: confinement
black brane
collapse
gravitation

References(66)

Figures(0)

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,
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,
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