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String Theory clues for the low-$\ell$ CMB ?

"Brane Supersymmetry Breaking" is a peculiar string-scale mechanism that can unpair Bose and Fermi excitations in orientifold models. It results from the simultaneous presence, in the vacuum, of collections of D-branes and orientifolds that are not mutually BPS, and is closely tied to the...

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Detalles Bibliográficos
Autores principales: Kitazawa, N., Sagnotti, A.
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:https://dx.doi.org/10.1051/epjconf/20159503031
http://cds.cern.ch/record/1971596
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author Kitazawa, N.
Sagnotti, A.
author_facet Kitazawa, N.
Sagnotti, A.
author_sort Kitazawa, N.
collection CERN
description "Brane Supersymmetry Breaking" is a peculiar string-scale mechanism that can unpair Bose and Fermi excitations in orientifold models. It results from the simultaneous presence, in the vacuum, of collections of D-branes and orientifolds that are not mutually BPS, and is closely tied to the scale of string excitations. It also leaves behind, for a mixing of dilaton and internal breathing mode, an exponential potential that is just too steep for a scalar to emerge from the initial singularity while descending it. As a result, in this class of models the scalar can generically bounce off the exponential wall, and this dynamics brings along, in the power spectrum, an infrared depression typically followed by a pre-inflationary peak. We elaborate on a possible link between this type of bounce and the low-$\ell$ end of the CMB angular power spectrum. For the first 32 multipoles, one can reach a 50 % reduction in $\chi^{\,2}$ with respect to the standard $\Lambda$CDM setting.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
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spelling cern-19715962022-08-10T13:02:52Zdoi:10.1051/epjconf/20159503031http://cds.cern.ch/record/1971596engKitazawa, N.Sagnotti, A.String Theory clues for the low-$\ell$ CMB ?Particle Physics - Theory"Brane Supersymmetry Breaking" is a peculiar string-scale mechanism that can unpair Bose and Fermi excitations in orientifold models. It results from the simultaneous presence, in the vacuum, of collections of D-branes and orientifolds that are not mutually BPS, and is closely tied to the scale of string excitations. It also leaves behind, for a mixing of dilaton and internal breathing mode, an exponential potential that is just too steep for a scalar to emerge from the initial singularity while descending it. As a result, in this class of models the scalar can generically bounce off the exponential wall, and this dynamics brings along, in the power spectrum, an infrared depression typically followed by a pre-inflationary peak. We elaborate on a possible link between this type of bounce and the low-$\ell$ end of the CMB angular power spectrum. For the first 32 multipoles, one can reach a 50 % reduction in $\chi^{\,2}$ with respect to the standard $\Lambda$CDM setting."Brane Supersymmetry Breaking" is a peculiar string-scale mechanism that can unpair Bose and Fermi excitations in orientifold models. It results from the simultaneous presence, in the vacuum, of collections of D-branes and orientifolds that are not mutually BPS, and is closely tied to the scale of string excitations. It also leaves behind, for a mixing of dilaton and internal breathing mode, an exponential potential that is just too steep for a scalar to emerge from the initial singularity while descending it. As a result, in this class of models the scalar can generically bounce off the exponential wall, and this dynamics brings along, in the power spectrum, an infrared depression typically followed by a pre-inflationary peak. We elaborate on a possible link between this type of bounce and the low-$\ell$ end of the CMB angular power spectrum. For the first 32 multipoles, one can reach a 50 % reduction in $\chi^{\,2}$ with respect to the standard $\Lambda$CDM setting.'Brane Supersymmetry Breaking' is a peculiar string-scale mechanism that can unpair Bose and Fermi excitations in orientifold models. It results from the simultaneous presence, in the vacuum, of collections of D-branes and orientifolds that are not mutually BPS, and is closely tied to the scale of string excitations. It also leaves behind, for a mixing of dilaton and internal breathing mode, an exponential potential that is just too steep for a scalar to emerge from the initial singularity while descending it. As a result, in this class of models the scalar can generically bounce off the exponential wall, and this dynamics brings along, in the power spectrum, an infrared depression typically followed by a pre-inflationary peak. We elaborate on a possible link between this type of bounce and the low-l end of the CMB angular power spectrum. For the first 32 multipoles, one can reach a 50% reduction in chi^2 with respect to the standard LambdaCDM setting.arXiv:1411.6396oai:cds.cern.ch:19715962014-11-24
spellingShingle Particle Physics - Theory
Kitazawa, N.
Sagnotti, A.
String Theory clues for the low-$\ell$ CMB ?
title String Theory clues for the low-$\ell$ CMB ?
title_full String Theory clues for the low-$\ell$ CMB ?
title_fullStr String Theory clues for the low-$\ell$ CMB ?
title_full_unstemmed String Theory clues for the low-$\ell$ CMB ?
title_short String Theory clues for the low-$\ell$ CMB ?
title_sort string theory clues for the low-$\ell$ cmb ?
topic Particle Physics - Theory
url https://dx.doi.org/10.1051/epjconf/20159503031
http://cds.cern.ch/record/1971596
work_keys_str_mv AT kitazawan stringtheorycluesforthelowellcmb
AT sagnottia stringtheorycluesforthelowellcmb