Inflationary gravitational waves in collapse scheme models
The inflationary paradigm is an important cornerstone of the concordance cosmological model. However, standard inflation cannot fully address the transition from an early homogeneous and isotropic stage, to another one lacking such symmetries corresponding to our present universe. In previous works,...
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paper:paper_03702693_v752_n_p344_Mariani2023-06-08T15:37:21Z Inflationary gravitational waves in collapse scheme models Bengochea, Gabriel Roman Collapse schemes Cosmology Gravitational waves Inflation The inflationary paradigm is an important cornerstone of the concordance cosmological model. However, standard inflation cannot fully address the transition from an early homogeneous and isotropic stage, to another one lacking such symmetries corresponding to our present universe. In previous works, a self-induced collapse of the wave function has been suggested as the missing ingredient of inflation. Most of the analysis regarding the collapse hypothesis has been solely focused on the characteristics of the spectrum associated to scalar perturbations, and within a semiclassical gravity framework. In this Letter, working in terms of a joint metric-matter quantization for inflation, we calculate, for the first time, the tensor power spectrum and the tensor-to-scalar ratio corresponding to the amplitude of primordial gravitational waves resulting from considering a generic self-induced collapse. © 2015 The Authors. Fil:Bengochea, G.R. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2016 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v752_n_p344_Mariani http://hdl.handle.net/20.500.12110/paper_03702693_v752_n_p344_Mariani |
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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) |
topic |
Collapse schemes Cosmology Gravitational waves Inflation |
spellingShingle |
Collapse schemes Cosmology Gravitational waves Inflation Bengochea, Gabriel Roman Inflationary gravitational waves in collapse scheme models |
topic_facet |
Collapse schemes Cosmology Gravitational waves Inflation |
description |
The inflationary paradigm is an important cornerstone of the concordance cosmological model. However, standard inflation cannot fully address the transition from an early homogeneous and isotropic stage, to another one lacking such symmetries corresponding to our present universe. In previous works, a self-induced collapse of the wave function has been suggested as the missing ingredient of inflation. Most of the analysis regarding the collapse hypothesis has been solely focused on the characteristics of the spectrum associated to scalar perturbations, and within a semiclassical gravity framework. In this Letter, working in terms of a joint metric-matter quantization for inflation, we calculate, for the first time, the tensor power spectrum and the tensor-to-scalar ratio corresponding to the amplitude of primordial gravitational waves resulting from considering a generic self-induced collapse. © 2015 The Authors. |
author |
Bengochea, Gabriel Roman |
author_facet |
Bengochea, Gabriel Roman |
author_sort |
Bengochea, Gabriel Roman |
title |
Inflationary gravitational waves in collapse scheme models |
title_short |
Inflationary gravitational waves in collapse scheme models |
title_full |
Inflationary gravitational waves in collapse scheme models |
title_fullStr |
Inflationary gravitational waves in collapse scheme models |
title_full_unstemmed |
Inflationary gravitational waves in collapse scheme models |
title_sort |
inflationary gravitational waves in collapse scheme models |
publishDate |
2016 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v752_n_p344_Mariani http://hdl.handle.net/20.500.12110/paper_03702693_v752_n_p344_Mariani |
work_keys_str_mv |
AT bengocheagabrielroman inflationarygravitationalwavesincollapseschememodels |
_version_ |
1768543183659073536 |