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Minimal Inflation

Using the universal X superfield that measures in the UV the violation of conformal invariance we build up a model of multifield inflation. The underlying dynamics is the one controlling the natural flow of this field in the IR to the Goldstino superfield once SUSY is broken. We show that flat direc...

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Detalles Bibliográficos
Autores principales: Alvarez-Gaume, Luis, Gomez, Cesar, Jimenez, Raul
Formato: info:eu-repo/semantics/article
Lenguaje:eng
Publicado: Phys. Lett. B 2010
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.physletb.2010.04.069
http://cds.cern.ch/record/1231387
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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 Using the universal X superfield that measures in the UV the violation of conformal invariance we build up a model of multifield inflation. The underlying dynamics is the one controlling the natural flow of this field in the IR to the Goldstino superfield once SUSY is broken. We show that flat directions satisfying the slow roll conditions exist only if R-symmetry is broken. Naturalness of our model leads to scales of SUSY breaking of the order of 10^{11-13} Gev, a nearly scale-invariant spectrum of the initial perturbations and negligible gravitational waves. We obtain that the inflaton field is lighter than the gravitino by an amount determined by the slow roll parameter eta. The existence of slow-roll conditions is directly linked to the values of supersymmetry and R-symmetry breaking scales. We make cosmological predictions of our model and compare them to current data.
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spelling cern-12313872023-03-15T19:11:51Z doi:10.1016/j.physletb.2010.04.069 http://cds.cern.ch/record/1231387 eng Alvarez-Gaume, Luis Gomez, Cesar Jimenez, Raul Minimal Inflation Particle Physics - Theory Using the universal X superfield that measures in the UV the violation of conformal invariance we build up a model of multifield inflation. The underlying dynamics is the one controlling the natural flow of this field in the IR to the Goldstino superfield once SUSY is broken. We show that flat directions satisfying the slow roll conditions exist only if R-symmetry is broken. Naturalness of our model leads to scales of SUSY breaking of the order of 10^{11-13} Gev, a nearly scale-invariant spectrum of the initial perturbations and negligible gravitational waves. We obtain that the inflaton field is lighter than the gravitino by an amount determined by the slow roll parameter eta. The existence of slow-roll conditions is directly linked to the values of supersymmetry and R-symmetry breaking scales. We make cosmological predictions of our model and compare them to current data. Using the universal X -superfield that measures in the UV the violation of conformal invariance we build up a model of multifield inflation. The underlying dynamics is the one controlling the natural flow of this field in the IR to the goldstino superfield once SUSY is broken. We show that flat directions satisfying the slow-roll conditions exist only if R -symmetry is broken. Naturalness of our model leads to scales of SUSY breaking of the order of 10 11–13 GeV, a nearly scale-invariant spectrum of the initial perturbations and negligible gravitational waves. We obtain that the inflaton field is lighter than the gravitino by an amount determined by the slow-roll parameter η . The existence of slow-roll conditions is directly linked to the values of supersymmetry and R -symmetry breaking scales. We make cosmological predictions of our model and compare them to current data. Using the universal X superfield that measures in the UV the violation of conformal invariance we build up a model of multifield inflation. The underlying dynamics is the one controlling the natural flow of this field in the IR to the Goldstino superfield once SUSY is broken. We show that flat directions satisfying the slow roll conditions exist only if R-symmetry is broken. Naturalness of our model leads to scales of SUSY breaking of the order of 10^{11-13} Gev, a nearly scale-invariant spectrum of the initial perturbations and negligible gravitational waves. We obtain that the inflaton field is lighter than the gravitino by an amount determined by the slow roll parameter eta. The existence of slow-roll conditions is directly linked to the values of supersymmetry and R-symmetry breaking scales. We make cosmological predictions of our model and compare them to current data. info:eu-repo/grantAgreement/EC/FP7/237920 info:eu-repo/semantics/openAccess Education Level info:eu-repo/semantics/article http://cds.cern.ch/record/1231387 Phys. Lett. B Phys. Lett. B, (2010) pp. 68-72 2010-01-05
spellingShingle Particle Physics - Theory
Alvarez-Gaume, Luis
Gomez, Cesar
Jimenez, Raul
Minimal Inflation
title Minimal Inflation
title_full Minimal Inflation
title_fullStr Minimal Inflation
title_full_unstemmed Minimal Inflation
title_short Minimal Inflation
title_sort minimal inflation
topic Particle Physics - Theory
url https://dx.doi.org/10.1016/j.physletb.2010.04.069
http://cds.cern.ch/record/1231387
http://cds.cern.ch/record/1231387
work_keys_str_mv AT alvarezgaumeluis minimalinflation
AT gomezcesar minimalinflation
AT jimenezraul minimalinflation