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Quasinormal modes and holography

Abstract:
Quasinormal frequencies of electromagnetic and gravitational perturbations in asymptotically anti-de Sitter spacetime can be identified with poles of the corresponding real-time Green's functions in a holographically dual finite temperature field theory. The quasinormal modes are defined for gauge-invariant quantities which obey an incoming-wave boundary condition at the horizon and a Dirichlet condition at the boundary. As an application, we explicitly find poles of retarded correlation functions of R-symmetry currents and the energy-momentum tensor in strongly coupled finite temperature N=4 supersymmetric SU(Nc) Yang-Mills theory in the limit of large Nc. © 2005 The American Physical Society.

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Publisher copy:
10.1103/PhysRevD.72.086009

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Journal:
Physical Review D More from this journal
Volume:
72
Issue:
8
Publication date:
2005-10-15
DOI:
EISSN:
1550-2368
ISSN:
1550-7998


Language:
English
Pubs id:
pubs:160061
UUID:
uuid:b232a89c-aab1-4453-9697-f808a0801f77
Local pid:
pubs:160061
Source identifiers:
160061
Deposit date:
2012-12-19

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