Primordial gravitational waves and the collapse of the wave function

The self-induced collapse hypothesis was introduced by D. Sudarsky and collaborators to explain the origin of cosmic structure from a perfect isotropic and homogeneous universe during the inflationary regime. In this paper, we calculate the power spectrum for the tensor modes, within the semiclassic...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: León, G., Kraiselburd, L., Landau, S.J.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_15507998_v92_n8_p_Leon
Aporte de:
id todo:paper_15507998_v92_n8_p_Leon
record_format dspace
spelling todo:paper_15507998_v92_n8_p_Leon2023-10-03T16:25:16Z Primordial gravitational waves and the collapse of the wave function León, G. Kraiselburd, L. Landau, S.J. The self-induced collapse hypothesis was introduced by D. Sudarsky and collaborators to explain the origin of cosmic structure from a perfect isotropic and homogeneous universe during the inflationary regime. In this paper, we calculate the power spectrum for the tensor modes, within the semiclassical gravity approximation, with the additional hypothesis of a generic self-induced collapse of the inflaton's wave function; we also compute an estimate for the tensor-to-scalar ratio. Based on this calculation, we show that the considered proposal exhibits a strong suppression of the tensor modes amplitude; nevertheless, the corresponding amplitude is still consistent with the joint BICEP/KECK and Planck Collaboration's limit on the tensor-to-scalar ratio. © 2015 American Physical Society. Fil:Landau, S.J. 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_15507998_v92_n8_p_Leon
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 self-induced collapse hypothesis was introduced by D. Sudarsky and collaborators to explain the origin of cosmic structure from a perfect isotropic and homogeneous universe during the inflationary regime. In this paper, we calculate the power spectrum for the tensor modes, within the semiclassical gravity approximation, with the additional hypothesis of a generic self-induced collapse of the inflaton's wave function; we also compute an estimate for the tensor-to-scalar ratio. Based on this calculation, we show that the considered proposal exhibits a strong suppression of the tensor modes amplitude; nevertheless, the corresponding amplitude is still consistent with the joint BICEP/KECK and Planck Collaboration's limit on the tensor-to-scalar ratio. © 2015 American Physical Society.
format JOUR
author León, G.
Kraiselburd, L.
Landau, S.J.
spellingShingle León, G.
Kraiselburd, L.
Landau, S.J.
Primordial gravitational waves and the collapse of the wave function
author_facet León, G.
Kraiselburd, L.
Landau, S.J.
author_sort León, G.
title Primordial gravitational waves and the collapse of the wave function
title_short Primordial gravitational waves and the collapse of the wave function
title_full Primordial gravitational waves and the collapse of the wave function
title_fullStr Primordial gravitational waves and the collapse of the wave function
title_full_unstemmed Primordial gravitational waves and the collapse of the wave function
title_sort primordial gravitational waves and the collapse of the wave function
url http://hdl.handle.net/20.500.12110/paper_15507998_v92_n8_p_Leon
work_keys_str_mv AT leong primordialgravitationalwavesandthecollapseofthewavefunction
AT kraiselburdl primordialgravitationalwavesandthecollapseofthewavefunction
AT landausj primordialgravitationalwavesandthecollapseofthewavefunction
_version_ 1807319324094889984