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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Autores principales: Harari, Diego Darío, Mazzitelli, Francisco Diego
Publicado: 1990
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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spelling 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
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