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A Simple No-Scale Model of Modulus Fixing and Inflation

We construct a no-scale model of inflation with a single modulus whose real and imaginary parts are fixed by simple power-law corrections to the no-scale Kähler potential. Assuming an uplift of the minimum of the effective potential, the model yields a suitable number of e-folds of expansion and val...

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Detalles Bibliográficos
Autores principales: Ellis, John, Fairbairn, Malcolm, Romano, Antonio Enea, Zapata, Óscar
Lenguaje:eng
Publicado: 2018
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.98.103514
http://cds.cern.ch/record/2305780
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author Ellis, John
Fairbairn, Malcolm
Romano, Antonio Enea
Zapata, Óscar
author_facet Ellis, John
Fairbairn, Malcolm
Romano, Antonio Enea
Zapata, Óscar
author_sort Ellis, John
collection CERN
description We construct a no-scale model of inflation with a single modulus whose real and imaginary parts are fixed by simple power-law corrections to the no-scale Kähler potential. Assuming an uplift of the minimum of the effective potential, the model yields a suitable number of e-folds of expansion and values of the tilt in the scalar cosmological density perturbations and of the ratio of tensor and scalar perturbations that are compatible with measurements of the cosmic microwave background radiation.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2018
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spelling cern-23057802020-06-23T10:28:01Zdoi:10.1103/PhysRevD.98.103514http://cds.cern.ch/record/2305780engEllis, JohnFairbairn, MalcolmRomano, Antonio EneaZapata, ÓscarA Simple No-Scale Model of Modulus Fixing and Inflationhep-thParticle Physics - Theorygr-qcGeneral Relativity and Cosmologyastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyWe construct a no-scale model of inflation with a single modulus whose real and imaginary parts are fixed by simple power-law corrections to the no-scale Kähler potential. Assuming an uplift of the minimum of the effective potential, the model yields a suitable number of e-folds of expansion and values of the tilt in the scalar cosmological density perturbations and of the ratio of tensor and scalar perturbations that are compatible with measurements of the cosmic microwave background radiation.We construct a no-scale model of inflation with a single modulus whose real and imaginary parts are fixed by simple power-law corrections to the no-scale K{\" a}hler potential. Assuming an uplift of the minimum of the effective potential, the model yields a suitable number of e-folds of expansion and values of the tilt in the scalar cosmological density perturbations and of the ratio of tensor and scalar perturbations that are compatible with measurements of the cosmic microwave background radiation.arXiv:1802.05713KCL-PH-TH-2018-05CERN-PH-TH-2018-028CERN-TH-2018-028KCL-PH-TH/2018-05CERN-PH-TH/2018-028oai:cds.cern.ch:23057802018-02-15
spellingShingle hep-th
Particle Physics - Theory
gr-qc
General Relativity and Cosmology
astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
Ellis, John
Fairbairn, Malcolm
Romano, Antonio Enea
Zapata, Óscar
A Simple No-Scale Model of Modulus Fixing and Inflation
title A Simple No-Scale Model of Modulus Fixing and Inflation
title_full A Simple No-Scale Model of Modulus Fixing and Inflation
title_fullStr A Simple No-Scale Model of Modulus Fixing and Inflation
title_full_unstemmed A Simple No-Scale Model of Modulus Fixing and Inflation
title_short A Simple No-Scale Model of Modulus Fixing and Inflation
title_sort simple no-scale model of modulus fixing and inflation
topic hep-th
Particle Physics - Theory
gr-qc
General Relativity and Cosmology
astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.98.103514
http://cds.cern.ch/record/2305780
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