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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...
Autores principales: | , |
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Lenguaje: | eng |
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2014
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Acceso en línea: | https://dx.doi.org/10.1051/epjconf/20159503031 http://cds.cern.ch/record/1971596 |
_version_ | 1780944856371167232 |
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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. |
id | cern-1971596 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2014 |
record_format | invenio |
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 |