Reassessing the link between B-modes and inflation
We reevaluate the predictions of inflation regarding primordial gravity waves, which should appear as B-modes in the cosmic microwave background (CMB), in light of the fact that the standard inflationary paradigm is unable to account for the transition from an initially symmetric state into a nonsym...
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Autores principales: | , , , |
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Formato: | Articulo Preprint |
Lenguaje: | Inglés |
Publicado: |
2017
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/125598 |
Aporte de: |
id |
I19-R120-10915-125598 |
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record_format |
dspace |
institution |
Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Física Big bang Physics Statistical physics Primordial fluctuations Gravitational wave Inflation (cosmology) Cosmic microwave background Asymmetry Astrophysics Collapse (topology) Cosmic background radiation |
spellingShingle |
Física Big bang Physics Statistical physics Primordial fluctuations Gravitational wave Inflation (cosmology) Cosmic microwave background Asymmetry Astrophysics Collapse (topology) Cosmic background radiation León, Gabriel Majhi, Abhishek Okon, Elias Sudarsky, Daniel Reassessing the link between B-modes and inflation |
topic_facet |
Física Big bang Physics Statistical physics Primordial fluctuations Gravitational wave Inflation (cosmology) Cosmic microwave background Asymmetry Astrophysics Collapse (topology) Cosmic background radiation |
description |
We reevaluate the predictions of inflation regarding primordial gravity waves, which should appear as B-modes in the cosmic microwave background (CMB), in light of the fact that the standard inflationary paradigm is unable to account for the transition from an initially symmetric state into a nonsymmetric outcome. We show that the incorporation of an element capable of explaining such a transition dramatically alters the prediction for the shape and size of the B-mode spectrum. In particular, we find that by adapting a realistic objective collapse model to the situation at hand, the B-mode spectrum becomes strongly suppressed with respect to the standard prediction. We conclude that the failure to detect B-modes in the CMB does not rule out the simplest inflationary models. |
format |
Articulo Preprint |
author |
León, Gabriel Majhi, Abhishek Okon, Elias Sudarsky, Daniel |
author_facet |
León, Gabriel Majhi, Abhishek Okon, Elias Sudarsky, Daniel |
author_sort |
León, Gabriel |
title |
Reassessing the link between B-modes and inflation |
title_short |
Reassessing the link between B-modes and inflation |
title_full |
Reassessing the link between B-modes and inflation |
title_fullStr |
Reassessing the link between B-modes and inflation |
title_full_unstemmed |
Reassessing the link between B-modes and inflation |
title_sort |
reassessing the link between b-modes and inflation |
publishDate |
2017 |
url |
http://sedici.unlp.edu.ar/handle/10915/125598 |
work_keys_str_mv |
AT leongabriel reassessingthelinkbetweenbmodesandinflation AT majhiabhishek reassessingthelinkbetweenbmodesandinflation AT okonelias reassessingthelinkbetweenbmodesandinflation AT sudarskydaniel reassessingthelinkbetweenbmodesandinflation |
bdutipo_str |
Repositorios |
_version_ |
1764820451927785475 |