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Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5)

We embed a flipped SU(5) × U(1) GUT model in a no-scale supergravity framework, and discuss its predictions for cosmic microwave background observables, which are similar to those of the Starobinsky model of inflation. Measurements of the tilt in the spectrum of scalar perturbations in the cosmic mi...

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Detalles Bibliográficos
Autores principales: Ellis, John, Garcia, Marcos A. G., Nagata, Natsumi, Nanopoulos, Dimitri V., Olive, Keith A.
Lenguaje:eng
Publicado: 2017
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2017/07/006
http://cds.cern.ch/record/2261145
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author Ellis, John
Garcia, Marcos A. G.
Nagata, Natsumi
Nanopoulos, Dimitri V.
Olive, Keith A.
author_facet Ellis, John
Garcia, Marcos A. G.
Nagata, Natsumi
Nanopoulos, Dimitri V.
Olive, Keith A.
author_sort Ellis, John
collection CERN
description We embed a flipped SU(5) × U(1) GUT model in a no-scale supergravity framework, and discuss its predictions for cosmic microwave background observables, which are similar to those of the Starobinsky model of inflation. Measurements of the tilt in the spectrum of scalar perturbations in the cosmic microwave background, ns, constrain significantly the model parameters. We also discuss the model's predictions for neutrino masses, and pay particular attention to the behaviours of scalar fields during and after inflation, reheating and the GUT phase transition. We argue in favor of strong reheating in order to avoid excessive entropy production which could dilute the generated baryon asymmetry.
id cern-2261145
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2017
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spelling cern-22611452023-09-12T03:12:17Zdoi:10.1088/1475-7516/2017/07/006http://cds.cern.ch/record/2261145engEllis, JohnGarcia, Marcos A. G.Nagata, NatsumiNanopoulos, Dimitri V.Olive, Keith A.Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5)hep-thParticle Physics - Theorygr-qcGeneral Relativity and Cosmologyastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyWe embed a flipped SU(5) × U(1) GUT model in a no-scale supergravity framework, and discuss its predictions for cosmic microwave background observables, which are similar to those of the Starobinsky model of inflation. Measurements of the tilt in the spectrum of scalar perturbations in the cosmic microwave background, ns, constrain significantly the model parameters. We also discuss the model's predictions for neutrino masses, and pay particular attention to the behaviours of scalar fields during and after inflation, reheating and the GUT phase transition. We argue in favor of strong reheating in order to avoid excessive entropy production which could dilute the generated baryon asymmetry.We embed a flipped ${\rm SU}(5) \times {\rm U}(1)$ GUT model in a no-scale supergravity framework, and discuss its predictions for cosmic microwave background observables, which are similar to those of the Starobinsky model of inflation. Measurements of the tilt in the spectrum of scalar perturbations in the cosmic microwave background, $n_s$, constrain significantly the model parameters. We also discuss the model's predictions for neutrino masses, and pay particular attention to the behaviours of scalar fields during and after inflation, reheating and the GUT phase transition. We argue in favor of strong reheating in order to avoid excessive entropy production which could dilute the generated baryon asymmetry.arXiv:1704.07331KCL-PH-TH-2017-17CERN-PH-TH-2017-071CERN-TH-2017-071UT-17-16ACT-03-17UMN-TH-3623-17FTPI-MINN-17-08MI-TH-1752oai:cds.cern.ch:22611452017-04-24
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
Garcia, Marcos A. G.
Nagata, Natsumi
Nanopoulos, Dimitri V.
Olive, Keith A.
Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5)
title Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5)
title_full Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5)
title_fullStr Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5)
title_full_unstemmed Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5)
title_short Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5)
title_sort starobinsky-like inflation, supercosmology and neutrino masses in no-scale flipped su(5)
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/10.1088/1475-7516/2017/07/006
http://cds.cern.ch/record/2261145
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