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Report/Contribution to a conference proceedings/Contribution to a book | PUBDB-2018-01776 |
2018
Verlag Deutsches Elektronen-Synchrotron
Hamburg
ISBN: 978-3-945931-17-2
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2017-02/saikawa_kenichi
Report No.: DESY-PROC-2017-02
Abstract: In this contribution, we highlight a problem in estimation of the mass of axion dark matter in the scenario where the Peccei-Quinn symmetry is broken after inflation. In order to obtain a definite prediction for its mass, it is necessary to evaluate its relic abundance precisely by taking account of the production from cosmic strings and domain walls. After reviewing a long-standing controversy about the axion production efficiency from decaying strings, several recent approaches aiming at resolving the uncertainty are discussed.
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Book/Proceedings/Report
13th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2017
13th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2017, ThessalonikiThessaloniki, Greece, 15 May 2017 - 19 May 2017
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC (2018) [10.3204/DESY-PROC-2017-02]
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