Quasinormal modes of a semi-holographic black brane and thermalization

被引:7
|
作者
Mondkar, Sukrut [1 ]
Mukhopadhyay, Ayan [1 ]
Rebhan, Anton [2 ]
Soloviev, Alexander [3 ]
机构
[1] Indian Inst Technol Madras, Ctr Strings Gravitat & Cosmol, Dept Phys, Chennai 600036, Tamil Nadu, India
[2] Tech Univ Wien, Inst Theoret Phys, Wiedner Hauptstr 8-10, A-1040 Vienna, Austria
[3] SUNY Stony Brook, Dept Phys & Astron, Ctr Nucl Theory, Stony Brook, NY 11794 USA
基金
奥地利科学基金会;
关键词
Gauge-gravity correspondence; Black Holes; Holography and quark-gluon plasmas;
D O I
10.1007/JHEP11(2021)080
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study the quasinormal modes and non-linear dynamics of a simplified model of semi-holography, which consistently integrates mutually interacting perturbative and strongly coupled holographic degrees of freedom such that the full system has a total conserved energy. We show that the thermalization of the full system can be parametrically slow when the mutual coupling is weak. For typical homogeneous initial states, we find that initially energy is transferred from the black brane to the perturbative sector, later giving way to complete transfer of energy to the black brane at a slow and constant rate, while the entropy grows monotonically for all time. Larger mutual coupling between the two sectors leads to larger extraction of energy from the black brane by the boundary perturbative system, but also quicker irreversible transfer of energy back to the black brane. The quasinormal modes replicate features of a dissipative system with a softly broken symmetry including the so-called k-gap. Furthermore, when the mutual coupling is below a critical value, there exists a hybrid zero mode with finite momentum which becomes unstable at higher values of momentum, indicating a Gregory-Laflamme type instability. This could imply turbulent equipartitioning of energy between the boundary and the holographic degrees of freedom in the presence of inhomogeneities.
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页数:41
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