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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...

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Detalles Bibliográficos
Autores principales: Alvarez-Gaume, Luis, Gomez, Cesar, Jimenez, Raul
Lenguaje:eng
Publicado: 2011
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2012/03/017
http://cds.cern.ch/record/1391957
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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.
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institution Organización Europea para la Investigación Nuclear
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publishDate 2011
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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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AT gomezcesar phenomenologyoftheminimalinflationscenarioinflationarytrajectoriesandparticleproduction
AT jimenezraul phenomenologyoftheminimalinflationscenarioinflationarytrajectoriesandparticleproduction