Relaxing isocurvature bounds on string axion dark matter
If inflation scale is high, light scalars acquire large quantum fluctuations during inflation. If sufficiently long-lived, they will give rise to CDM isocurvature perturbations, which are highly constrained by the Planck data. Focusing on string axions as such light scalars, we show that thermal inf...
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doaj-e85789b39a154dbf8ed7bb0dbba0cbe92020-11-24T21:21:48ZengElsevierPhysics Letters B0370-26931873-24452014-10-01737C17818410.1016/j.physletb.2014.08.017Relaxing isocurvature bounds on string axion dark matterMasahiro Kawasaki0Naoya Kitajima1Fuminobu Takahashi2Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, JapanDepartment of Physics, Tohoku University, Sendai 980-8578, JapanDepartment of Physics, Tohoku University, Sendai 980-8578, JapanIf inflation scale is high, light scalars acquire large quantum fluctuations during inflation. If sufficiently long-lived, they will give rise to CDM isocurvature perturbations, which are highly constrained by the Planck data. Focusing on string axions as such light scalars, we show that thermal inflation can provide a sufficiently large entropy production to dilute the CDM isocurvature perturbations. Importantly, efficient dilution is possible for the string axions, because effectively no secondary coherent oscillations are induced at the end of thermal inflation, in contrast to the moduli fields. We also study the viability of the axion dark matter with mass of about 7 keV as the origin of the 3.5 keV X-ray line excess, in the presence of large entropy production.http://www.sciencedirect.com/science/article/pii/S037026931400584X |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Masahiro Kawasaki Naoya Kitajima Fuminobu Takahashi |
spellingShingle |
Masahiro Kawasaki Naoya Kitajima Fuminobu Takahashi Relaxing isocurvature bounds on string axion dark matter Physics Letters B |
author_facet |
Masahiro Kawasaki Naoya Kitajima Fuminobu Takahashi |
author_sort |
Masahiro Kawasaki |
title |
Relaxing isocurvature bounds on string axion dark matter |
title_short |
Relaxing isocurvature bounds on string axion dark matter |
title_full |
Relaxing isocurvature bounds on string axion dark matter |
title_fullStr |
Relaxing isocurvature bounds on string axion dark matter |
title_full_unstemmed |
Relaxing isocurvature bounds on string axion dark matter |
title_sort |
relaxing isocurvature bounds on string axion dark matter |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 1873-2445 |
publishDate |
2014-10-01 |
description |
If inflation scale is high, light scalars acquire large quantum fluctuations during inflation. If sufficiently long-lived, they will give rise to CDM isocurvature perturbations, which are highly constrained by the Planck data. Focusing on string axions as such light scalars, we show that thermal inflation can provide a sufficiently large entropy production to dilute the CDM isocurvature perturbations. Importantly, efficient dilution is possible for the string axions, because effectively no secondary coherent oscillations are induced at the end of thermal inflation, in contrast to the moduli fields. We also study the viability of the axion dark matter with mass of about 7 keV as the origin of the 3.5 keV X-ray line excess, in the presence of large entropy production. |
url |
http://www.sciencedirect.com/science/article/pii/S037026931400584X |
work_keys_str_mv |
AT masahirokawasaki relaxingisocurvatureboundsonstringaxiondarkmatter AT naoyakitajima relaxingisocurvatureboundsonstringaxiondarkmatter AT fuminobutakahashi relaxingisocurvatureboundsonstringaxiondarkmatter |
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1725998134118580224 |