Nontrivial dynamics in the early stages of inflation

Inflationary cosmologies, regarded as dynamical systems, have rather simple asymptotic behavior insofar as the cosmic baldness principle holds. Nevertheless, in the early stages of an inflationary process the dynamical behavior may be very complex. In this paper, we show how even a simple inflationa...

Descripción completa

Guardado en:
Detalles Bibliográficos
Publicado: 1995
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v51_n6_p2713_Calzetta
http://hdl.handle.net/20.500.12110/paper_05562821_v51_n6_p2713_Calzetta
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_05562821_v51_n6_p2713_Calzetta
record_format dspace
spelling paper:paper_05562821_v51_n6_p2713_Calzetta2023-06-08T15:42:17Z Nontrivial dynamics in the early stages of inflation Inflationary cosmologies, regarded as dynamical systems, have rather simple asymptotic behavior insofar as the cosmic baldness principle holds. Nevertheless, in the early stages of an inflationary process the dynamical behavior may be very complex. In this paper, we show how even a simple inflationary scenario, based on Linde's "chaotic inflation" proposal, manifests nontrivial dynamical effects such as the breakup of invariant tori, the formation of cantori, and Arnol'd's diffusion. The relevance of such effects is highlighted by the facts that even the occurrence or nonoccurrence of inflation in a given universe is dependent upon them. © 1995 The American Physical Society. 1995 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v51_n6_p2713_Calzetta http://hdl.handle.net/20.500.12110/paper_05562821_v51_n6_p2713_Calzetta
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description Inflationary cosmologies, regarded as dynamical systems, have rather simple asymptotic behavior insofar as the cosmic baldness principle holds. Nevertheless, in the early stages of an inflationary process the dynamical behavior may be very complex. In this paper, we show how even a simple inflationary scenario, based on Linde's "chaotic inflation" proposal, manifests nontrivial dynamical effects such as the breakup of invariant tori, the formation of cantori, and Arnol'd's diffusion. The relevance of such effects is highlighted by the facts that even the occurrence or nonoccurrence of inflation in a given universe is dependent upon them. © 1995 The American Physical Society.
title Nontrivial dynamics in the early stages of inflation
spellingShingle Nontrivial dynamics in the early stages of inflation
title_short Nontrivial dynamics in the early stages of inflation
title_full Nontrivial dynamics in the early stages of inflation
title_fullStr Nontrivial dynamics in the early stages of inflation
title_full_unstemmed Nontrivial dynamics in the early stages of inflation
title_sort nontrivial dynamics in the early stages of inflation
publishDate 1995
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v51_n6_p2713_Calzetta
http://hdl.handle.net/20.500.12110/paper_05562821_v51_n6_p2713_Calzetta
_version_ 1768544277810380800

Ejemplares similares