Symmetry and inflation
We find the group of symmetry transformations under which the Einstein equations for the spatially flat Friedmann-Robertson-Walker universe are form invariant. They relate the energy density and the pressure of the fluid to the expansion rate. We show that inflation can be obtained from nonaccelerat...
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todo:paper_05562821_v65_n6_p_Chimento2023-10-03T15:35:46Z Symmetry and inflation Chimento, L.P. anisotropy article cosmos mathematical analysis model space time We find the group of symmetry transformations under which the Einstein equations for the spatially flat Friedmann-Robertson-Walker universe are form invariant. They relate the energy density and the pressure of the fluid to the expansion rate. We show that inflation can be obtained from nonaccelerated scenarios by a symmetry transformation. We derive the transformation rule for the spectrum and spectral index of the curvature perturbations. Finally, the group is extended to investigate inflation in the anisotropic Bianchi type-I spacetime and the brane-world cosmology. © 2002 The American Physical Society. Fil:Chimento, L.P. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_05562821_v65_n6_p_Chimento |
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Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
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anisotropy article cosmos mathematical analysis model space time |
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anisotropy article cosmos mathematical analysis model space time Chimento, L.P. Symmetry and inflation |
topic_facet |
anisotropy article cosmos mathematical analysis model space time |
description |
We find the group of symmetry transformations under which the Einstein equations for the spatially flat Friedmann-Robertson-Walker universe are form invariant. They relate the energy density and the pressure of the fluid to the expansion rate. We show that inflation can be obtained from nonaccelerated scenarios by a symmetry transformation. We derive the transformation rule for the spectrum and spectral index of the curvature perturbations. Finally, the group is extended to investigate inflation in the anisotropic Bianchi type-I spacetime and the brane-world cosmology. © 2002 The American Physical Society. |
format |
JOUR |
author |
Chimento, L.P. |
author_facet |
Chimento, L.P. |
author_sort |
Chimento, L.P. |
title |
Symmetry and inflation |
title_short |
Symmetry and inflation |
title_full |
Symmetry and inflation |
title_fullStr |
Symmetry and inflation |
title_full_unstemmed |
Symmetry and inflation |
title_sort |
symmetry and inflation |
url |
http://hdl.handle.net/20.500.12110/paper_05562821_v65_n6_p_Chimento |
work_keys_str_mv |
AT chimentolp symmetryandinflation |
_version_ |
1807324127618400256 |