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| 001 | 315502 | ||
| 005 | 20211110140134.0 | ||
| 020 | _ | _ | |a 978-3-935702-59-1 |
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2014-03/davidson_sacha |2 datacite_doi |
| 024 | 7 | _ | |a 1435-8077 |2 ISSN |
| 037 | _ | _ | |a PUBDB-2016-05909 |
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| 100 | 1 | _ | |a Davidson, Sacha |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 10th Patras Workshop on Axions, WIMPs and WISPs |c Geneva |d 2014-06-29 - 2014-07-04 |g AXION-WIMP 2014 |0 C14-06-29.1 |2 inspire |w Switzerland |
| 245 | _ | _ | |a The Pressure of Misalignment Axions: a Difference from WIMPs in Galaxy Formation? |
| 260 | _ | _ | |a Hamburg |c 2014 |b Verlag Deutsches Elektronen-Synchrotron |
| 295 | 1 | 0 | |a Davidson, Sacha "The Pressure of Misalignment Axions:a Difference from WIMPs in Galaxy Formation?" in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva |
| 300 | _ | _ | |a 51-54 |
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| 520 | _ | _ | |a Two populations of axions can contribute to cold dark matter: the classical field produced via the misalignment mechanism, and the modes produced in the decay of strings. The classical field has extra pressure, as compared to WIMPs, which could have observable consequences in non-linear galaxy formation. |
| 787 | 0 | _ | |a Tsesmelis, Emmanuel et. al. |d Verlag Deutsches Elektronen-Synchrotron |i isPartOf |0 PUBDB-2016-05897 |r DESY-PROC-2014-03 |t Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) : Geneva, Switzerland, June 29-July 4, 2014 |
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