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Phenomenology of the minimal inflation scenario: inflationary trajectories and particle production
We discuss the phenomenology of the minimal inflation scenario. We concentrate on two aspects: inflationary trajectories and particle production. Our findings can be summarized in two main results: first, that inflationary trayectories that are very flat and provide enough number of e-foldings are v...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
2011
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Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2012/03/017 http://cds.cern.ch/record/1391957 |
_version_ | 1780923427338584064 |
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author | Alvarez-Gaume, Luis Gomez, Cesar Jimenez, Raul |
author_facet | Alvarez-Gaume, Luis Gomez, Cesar Jimenez, Raul |
author_sort | Alvarez-Gaume, Luis |
collection | CERN |
description | We discuss the phenomenology of the minimal inflation scenario. We concentrate on two aspects: inflationary trajectories and particle production. Our findings can be summarized in two main results: first, that inflationary trayectories that are very flat and provide enough number of e-foldings are very natural in the scenario without fine tunning. We present a general formalism to identify attractors in multi-field inflation regardless of trajectories fulfilling the slow-roll conditions. We then explore particle production in the model and show how the inflaton naturally transmutes into the current dark matter particle, thus providing a mechanism to identify the inflaton today: it is the dark matter. One interesting feature of our model is that it provides a novel mechanism to generate particles and entropy in the universe: the filling of the Fermi sphere up to a given momentum pF due to the sea of goldstinos that are an important part of the matter generated after inflation. With this mechanism in hand we predict that the gravitino should have a mass of > 100-1000 TeV. |
id | cern-1391957 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2011 |
record_format | invenio |
spelling | cern-13919572021-05-03T20:33:27Zdoi:10.1088/1475-7516/2012/03/017http://cds.cern.ch/record/1391957engAlvarez-Gaume, LuisGomez, CesarJimenez, RaulPhenomenology of the minimal inflation scenario: inflationary trajectories and particle productionAstrophysics and AstronomyWe discuss the phenomenology of the minimal inflation scenario. We concentrate on two aspects: inflationary trajectories and particle production. Our findings can be summarized in two main results: first, that inflationary trayectories that are very flat and provide enough number of e-foldings are very natural in the scenario without fine tunning. We present a general formalism to identify attractors in multi-field inflation regardless of trajectories fulfilling the slow-roll conditions. We then explore particle production in the model and show how the inflaton naturally transmutes into the current dark matter particle, thus providing a mechanism to identify the inflaton today: it is the dark matter. One interesting feature of our model is that it provides a novel mechanism to generate particles and entropy in the universe: the filling of the Fermi sphere up to a given momentum pF due to the sea of goldstinos that are an important part of the matter generated after inflation. With this mechanism in hand we predict that the gravitino should have a mass of > 100-1000 TeV.We discuss the phenomenology of the minimal inflation scenario. We concentrate on two aspects: inflationary trajectories and particle production. Our findings can be summarized in two main results: first, that inflationary trayectories that are very flat and provide enough number of e-foldings are natural in the scenario without fine tunning. We present a general formalism to identify attractors in multi-field inflation regardless of trajectories fulfilling the slow-roll conditions. We then explore particle production in the model and show how the inflaton naturally transmutes into a dark matter particle. One interesting feature of our model is that it provides a novel mechanism to generate particles and entropy in the universe: the filling of the Fermi sphere up to a given momentum p_F due to the sea of goldstinos that are an important part of the matter generated after inflation. With this mechanism in hand we predict that the gravitino should have a mass of > 100-1000 TeV. Another interesting feature of our model is that the predicted level of gravity waves is r=0.1 - 0.001, which is in the range of detectability from Planck and upcoming CMB polarization experiments.arXiv:1110.3984oai:cds.cern.ch:13919572011-10-19 |
spellingShingle | Astrophysics and Astronomy Alvarez-Gaume, Luis Gomez, Cesar Jimenez, Raul Phenomenology of the minimal inflation scenario: inflationary trajectories and particle production |
title | Phenomenology of the minimal inflation scenario: inflationary trajectories and particle production |
title_full | Phenomenology of the minimal inflation scenario: inflationary trajectories and particle production |
title_fullStr | Phenomenology of the minimal inflation scenario: inflationary trajectories and particle production |
title_full_unstemmed | Phenomenology of the minimal inflation scenario: inflationary trajectories and particle production |
title_short | Phenomenology of the minimal inflation scenario: inflationary trajectories and particle production |
title_sort | phenomenology of the minimal inflation scenario: inflationary trajectories and particle production |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1088/1475-7516/2012/03/017 http://cds.cern.ch/record/1391957 |
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