Quasinormal modes of brane-localized standard model fields

Journal Article · Wed Feb 15 04:00:00 EST 2006 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PhysRevD.73.044002· OSTI ID:20776740

Kanti, P; Konoplya, R A ^[1]

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1. Department of Mathematical Sciences, University of Durham, Science Site, South Road, Durham DH1 3LE (United Kingdom)

We present here a detailed study of the quasinormal spectrum of brane-localized standard model fields in the vicinity of D-dimensional black holes. A variety of such backgrounds [Schwarzschild, Reissner-Nordstroem and Schwarzszchild-(anti-)de Sitter] are investigated. The dependence of the quasinormal spectra on the dimensionality D, spin of the field s, and multipole number l is analyzed. Analytical formulas are obtained for a number of limiting cases: in the limit of large multipole number for Schwarzschild, Schwarzschild-de Sitter, and Reissner-Nordstroem black holes, in the extremal limit of the Schwarzschild-de Sitter black hole, and in the limit of small horizon radius in the case of Schwarzschild-anti-de Sitter black holes. We show that an increase in the number of hidden, extra dimensions results in the faster damping of all fields living on the brane, and that the localization of fields on a brane affects the quasinormal spectrum in a number of additional ways, both direct and indirect.

• OSTI ID: 20776740
• Journal Information: Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 4 Vol. 73; ISSN PRVDAQ; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
BLACK HOLES
COSMOLOGY
DAMPING
DE SITTER GROUP
ENERGY SPECTRA
MEMBRANES
SCHWARZSCHILD METRIC
SPACE-TIME
SPIN
STANDARD MODEL