# Quasinormal modes of brane-localized standard model fields

## Abstract

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.

- Authors:

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

- Publication Date:

- OSTI Identifier:
- 20776740

- Resource Type:
- Journal Article

- Resource Relation:
- Journal Name: Physical Review. D, Particles Fields; Journal Volume: 73; Journal Issue: 4; Other Information: DOI: 10.1103/PhysRevD.73.044002; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)

- Country of Publication:
- United States

- Language:
- English

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

### Citation Formats

```
Kanti, P., Konoplya, R.A., and Instituto de Fisica, Universidade de Sao Paulo, C.P. 66318, 05315-970, Sao Paulo-SP.
```*Quasinormal modes of brane-localized standard model fields*. United States: N. p., 2006.
Web. doi:10.1103/PhysRevD.73.044002.

```
Kanti, P., Konoplya, R.A., & Instituto de Fisica, Universidade de Sao Paulo, C.P. 66318, 05315-970, Sao Paulo-SP.
```*Quasinormal modes of brane-localized standard model fields*. United States. doi:10.1103/PhysRevD.73.044002.

```
Kanti, P., Konoplya, R.A., and Instituto de Fisica, Universidade de Sao Paulo, C.P. 66318, 05315-970, Sao Paulo-SP. Wed .
"Quasinormal modes of brane-localized standard model fields". United States.
doi:10.1103/PhysRevD.73.044002.
```

```
@article{osti_20776740,
```

title = {Quasinormal modes of brane-localized standard model fields},

author = {Kanti, P. and Konoplya, R.A. and Instituto de Fisica, Universidade de Sao Paulo, C.P. 66318, 05315-970, Sao Paulo-SP},

abstractNote = {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.},

doi = {10.1103/PhysRevD.73.044002},

journal = {Physical Review. D, Particles Fields},

number = 4,

volume = 73,

place = {United States},

year = {Wed Feb 15 00:00:00 EST 2006},

month = {Wed Feb 15 00:00:00 EST 2006}

}