A No-Scale Inflationary Model to Fit Them All

The magnitude of B-mode polarization in the cosmic microwave background as measured by BICEP2 favours models of chaotic inflation with a quadratic $m^2 \phi^2/2$ potential, whereas data from the Planck satellite favour a small value of the tensor-to-scalar perturbation ratio $r$ that is highly consi...

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Detalles Bibliográficos
Autores principales: Ellis, John, Garcia, Marcos A. G., Nanopoulos, Dimitri V., Olive, Keith A.
Publicado: 2014
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2014/08/044
http://cds.cern.ch/record/1697726
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author Ellis, John
Garcia, Marcos A. G.
Nanopoulos, Dimitri V.
Olive, Keith A.
author_facet Ellis, John
Garcia, Marcos A. G.
Nanopoulos, Dimitri V.
Olive, Keith A.
author_sort Ellis, John
collection CERN
description The magnitude of B-mode polarization in the cosmic microwave background as measured by BICEP2 favours models of chaotic inflation with a quadratic $m^2 \phi^2/2$ potential, whereas data from the Planck satellite favour a small value of the tensor-to-scalar perturbation ratio $r$ that is highly consistent with the Starobinsky $R + R^2$ model. Reality may lie somewhere between these two scenarios. In this paper we propose a minimal two-field no-scale supergravity model that interpolates between quadratic and Starobinsky-like inflation as limiting cases, while retaining the successful prediction $n_s \simeq 0.96$.
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institution Organización Europea para la Investigación Nuclear
publishDate 2014
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spelling cern-16977262023-03-14T19:23:27Zdoi:10.1088/1475-7516/2014/08/044http://cds.cern.ch/record/1697726Ellis, JohnGarcia, Marcos A. G.Nanopoulos, Dimitri V.Olive, Keith A.A No-Scale Inflationary Model to Fit Them AllParticle Physics - PhenomenologyThe magnitude of B-mode polarization in the cosmic microwave background as measured by BICEP2 favours models of chaotic inflation with a quadratic $m^2 \phi^2/2$ potential, whereas data from the Planck satellite favour a small value of the tensor-to-scalar perturbation ratio $r$ that is highly consistent with the Starobinsky $R + R^2$ model. Reality may lie somewhere between these two scenarios. In this paper we propose a minimal two-field no-scale supergravity model that interpolates between quadratic and Starobinsky-like inflation as limiting cases, while retaining the successful prediction $n_s \simeq 0.96$.The magnitude of B-mode polarization in the cosmic microwave background as measured by BICEP2 favours models of chaotic inflation with a quadratic m(2) phi(2)/2 potential, whereas data from the Planck satellite favour a small value of the tensor-to-scalar perturbation ratio r that is highly consistent with the Starobinsky R +R(2) model. Reality may lie somewhere between these two scenarios. In this paper we propose a minimal two-field no-scale supergravity model that interpolates between quadratic and Starobinsky-like inflation as limiting cases, while retaining the successful prediction ns simeq 0.96.The magnitude of B-mode polarization in the cosmic microwave background as measured by BICEP2 favours models of chaotic inflation with a quadratic $m^2 \phi^2/2$ potential, whereas data from the Planck satellite favour a small value of the tensor-to-scalar perturbation ratio $r$ that is highly consistent with the Starobinsky $R + R^2$ model. Reality may lie somewhere between these two scenarios. In this paper we propose a minimal two-field no-scale supergravity model that interpolates between quadratic and Starobinsky-like inflation as limiting cases, while retaining the successful prediction $n_s \simeq 0.96$.arXiv:1405.0271KCL-PH-TH-2014-18LCTS-2014-18CERN-PH-TH-2014-076ACT-5-14UMN-TH-3335-14FTPI-MINN-14-12KCL-PH-TH-2014-18LCTS-2014-18ACT-5-14UMN-TH-3335-14FTPI-MINN-14-12CERN-PH-TH-2014-076oai:cds.cern.ch:16977262014-04-29
spellingShingle Particle Physics - Phenomenology
Ellis, John
Garcia, Marcos A. G.
Nanopoulos, Dimitri V.
Olive, Keith A.
A No-Scale Inflationary Model to Fit Them All
title A No-Scale Inflationary Model to Fit Them All
title_full A No-Scale Inflationary Model to Fit Them All
title_fullStr A No-Scale Inflationary Model to Fit Them All
title_full_unstemmed A No-Scale Inflationary Model to Fit Them All
title_short A No-Scale Inflationary Model to Fit Them All
title_sort no-scale inflationary model to fit them all
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1088/1475-7516/2014/08/044
http://cds.cern.ch/record/1697726
work_keys_str_mv AT ellisjohn anoscaleinflationarymodeltofitthemall
AT garciamarcosag anoscaleinflationarymodeltofitthemall
AT nanopoulosdimitriv anoscaleinflationarymodeltofitthemall
AT olivekeitha anoscaleinflationarymodeltofitthemall
AT ellisjohn noscaleinflationarymodeltofitthemall
AT garciamarcosag noscaleinflationarymodeltofitthemall
AT nanopoulosdimitriv noscaleinflationarymodeltofitthemall
AT olivekeitha noscaleinflationarymodeltofitthemall

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