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| 001 | 408351 | ||
| 005 | 20211110151244.0 | ||
| 010 | _ | _ | |a |
| 020 | _ | _ | |a 978-3-935702-83-6 |
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2013-04/jeong_kwang_sik |2 datacite_doi |
| 024 | 7 | _ | |a 1435-8077 |2 ISSN |
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| 041 | _ | _ | |a English |
| 088 | 1 | _ | |a DESY-PROC-2013-04 |
| 088 | _ | _ | |a DESY-PROC-2013-04 |2 DESY |
| 100 | 1 | _ | |a Jeong, K. S. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 9th Patras Workshop on Axions, WIMPs and WISPs |c Mainz |d 2013-06-24 - 2013-06-28 |g AXION-WIMP 2013 |0 C13-06-24.5 |2 inspire |w Germany |
| 245 | _ | _ | |a Stronger QCD in the early Universe to suppress axion isocurvature perturbations |
| 260 | _ | _ | |a Hamburg |c 2013 |b Verlag Deutsches Elektronen-Synchrotron |
| 295 | 1 | 0 | |a Jeong, K.S. "Stronger QCD in the early Universe to suppress axion isocurvature perturbations" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz |
| 300 | _ | _ | |a 153-158 |
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| 490 | 0 | _ | |a DESY-PROC |0 PERI:(DE-600)2450075-6 |
| 520 | _ | _ | |a A stronger QCD in the early Universe renders the axion heavy, and thus can suppress the isocurvature perturbations of axion dark matter, relaxing the constraint on the inflation scale. Supersymmetry provides a natural framework for this because there is a flat direction involving Higgs fields. Stabilized at a large value during inflation, the Higgs flat direction leads to that the QCD interaction becomes strong at a high energy scale, making high scale inflation scenarios compatible with axion dark matter. |
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| 700 | 1 | _ | |a Takahashi, F. |0 P:(DE-HGF)0 |b 1 |
| 787 | 0 | _ | |a Oberlack, Uwe et. al. |0 PUBDB-2015-05816 |r DESY-PROC-2013-04 |i isPartOf |t Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) |
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