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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Detalles Bibliográficos
Autores principales:	Mariani, Mauro, Bengochea, Gabriel R., León, Gabriel
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2016
Materias:	Ciencias Astronómicas Collapse schemes Cosmology Gravitational waves Inflation
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85960
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

id	I19-R120-10915-85960
record_format	dspace
institution	Universidad Nacional de La Plata
institution_str	I-19
repository_str	R-120
collection	SEDICI (UNLP)
language	Inglés
topic	Ciencias Astronómicas Collapse schemes Cosmology Gravitational waves Inflation
spellingShingle	Ciencias Astronómicas Collapse schemes Cosmology Gravitational waves Inflation Mariani, Mauro Bengochea, Gabriel R. León, Gabriel Inflationary gravitational waves in collapse scheme models
topic_facet	Ciencias Astronómicas 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.
format	Articulo Articulo
author	Mariani, Mauro Bengochea, Gabriel R. León, Gabriel
author_facet	Mariani, Mauro Bengochea, Gabriel R. León, Gabriel
author_sort	Mariani, Mauro
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	http://sedici.unlp.edu.ar/handle/10915/85960
work_keys_str_mv	AT marianimauro inflationarygravitationalwavesincollapseschememodels AT bengocheagabrielr inflationarygravitationalwavesincollapseschememodels AT leongabriel inflationarygravitationalwavesincollapseschememodels
bdutipo_str	Repositorios
_version_	1764820489158524932

Inflationary gravitational waves in collapse scheme models

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