| Journal Article | PUBDB-2020-01572 |
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2020
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Please use a persistent id in citations: doi:10.1007/JHEP04(2020)010 doi:10.3204/PUBDB-2020-01572
Report No.: DESY-19-202; arXiv:1911.08472
Abstract: We investigate the production of axion quanta during the early universe evolution of an axion-like field rolling down a wiggly potential. We compute the growth of quantum fluctuations and their back-reaction on the homogeneous zero-mode. We evaluate the transfer of kinetic energy from the zero mode to the quantum fluctuations and the conditions to decelerate the axion zero-mode as a function of the Hubble rate, the slope of the potential, the size of the barriers and the initial field velocity. We discuss how these effects impact the relaxion mechanism.
Keyword(s): fluctuation: quantum ; axion: production ; potential: slope ; energy: kinetic ; zero mode ; Hubble constant ; fragmentation ; back reaction ; axion-like particles
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Preprint
Axion Fragmentation
[10.3204/PUBDB-2019-04368]
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