Conversion of Goldstone bosons into gravitons in anisotropic cosmology
The gravitational chiral anomaly makes possible the conversion of a Goldstone boson into a graviton in a background gravitational field. We show that the interaction Lagrangian for this process does not vanish if and only if the background metric has a nonvanishing Weyl tensor, i.e., if it is not co...
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1990
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v42_n8_p2632_Harari http://hdl.handle.net/20.500.12110/paper_05562821_v42_n8_p2632_Harari |
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paper:paper_05562821_v42_n8_p2632_Harari2023-06-08T15:42:09Z Conversion of Goldstone bosons into gravitons in anisotropic cosmology Harari, Diego Darío Mazzitelli, Francisco Diego The gravitational chiral anomaly makes possible the conversion of a Goldstone boson into a graviton in a background gravitational field. We show that the interaction Lagrangian for this process does not vanish if and only if the background metric has a nonvanishing Weyl tensor, i.e., if it is not conformally flat. No conversion takes place in an isotropic expanding universe. We evaluate the probability for the conversion of Goldstone bosons into gravitons in Bianchi type-I background metrics, the simplest anisotropic cosmological backgrounds. © 1990 The American Physical Society. Fil:Harari, D.D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Mazzitelli, F.D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 1990 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v42_n8_p2632_Harari http://hdl.handle.net/20.500.12110/paper_05562821_v42_n8_p2632_Harari |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
The gravitational chiral anomaly makes possible the conversion of a Goldstone boson into a graviton in a background gravitational field. We show that the interaction Lagrangian for this process does not vanish if and only if the background metric has a nonvanishing Weyl tensor, i.e., if it is not conformally flat. No conversion takes place in an isotropic expanding universe. We evaluate the probability for the conversion of Goldstone bosons into gravitons in Bianchi type-I background metrics, the simplest anisotropic cosmological backgrounds. © 1990 The American Physical Society. |
author |
Harari, Diego Darío Mazzitelli, Francisco Diego |
spellingShingle |
Harari, Diego Darío Mazzitelli, Francisco Diego Conversion of Goldstone bosons into gravitons in anisotropic cosmology |
author_facet |
Harari, Diego Darío Mazzitelli, Francisco Diego |
author_sort |
Harari, Diego Darío |
title |
Conversion of Goldstone bosons into gravitons in anisotropic cosmology |
title_short |
Conversion of Goldstone bosons into gravitons in anisotropic cosmology |
title_full |
Conversion of Goldstone bosons into gravitons in anisotropic cosmology |
title_fullStr |
Conversion of Goldstone bosons into gravitons in anisotropic cosmology |
title_full_unstemmed |
Conversion of Goldstone bosons into gravitons in anisotropic cosmology |
title_sort |
conversion of goldstone bosons into gravitons in anisotropic cosmology |
publishDate |
1990 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v42_n8_p2632_Harari http://hdl.handle.net/20.500.12110/paper_05562821_v42_n8_p2632_Harari |
work_keys_str_mv |
AT hararidiegodario conversionofgoldstonebosonsintogravitonsinanisotropiccosmology AT mazzitellifranciscodiego conversionofgoldstonebosonsintogravitonsinanisotropiccosmology |
_version_ |
1768545560646647808 |