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Journal Article | PUBDB-2024-00150 |
;
2023
American Physical Society
Ridge, NY
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Please use a persistent id in citations: doi:10.1103/PhysRevD.108.123516 doi:10.3204/PUBDB-2024-00150
Report No.: DESY-23-094; arXiv:2307.03121
Abstract: Models that produce Axion-Like-Particles (ALP) after cosmological inflation due to spontaneous $U(1)$ symmetry breaking also produce cosmic string networks. Those axionic strings lose energy through gravitational wave emission during the whole cosmological history, generating a stochastic background of gravitational waves that spans many decades in frequency. We can therefore constrain the axion decay constant and axion mass from limits on the gravitational wave spectrum and compatibility with dark matter abundance as well as dark radiation. We derive such limits from analyzing the most recent NANOGrav data from Pulsar Timing Arrays (PTA). The limits are compatible with the slightly stronger $N_{\rm eff}$ bounds on dark radiation for ALP masses $m_a \lesssim 10^{-10}$ eV. On the other hand, for heavy ALPs with $m_a\gtrsim 0.1$ GeV and $N_{\rm DW}\neq 1$, new regions of parameter space can be probed by PTA data due to the dominant Domain-Wall contribution to the gravitational wave background.
Keyword(s): gravitational radiation: background ; cosmic string: network ; axion: decay constant ; axion: string ; gravitational radiation: spectrum ; axion: mass ; background: stochastic ; gravitational radiation: emission ; dark matter: parametrization ; pulsar ; symmetry: U(1) ; domain wall ; NANOGrav ; inflation: model ; symmetry breaking ; axion-like particles ; history
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Preprint
Constraining Post-Inflationary Axions with Pulsar Timing Arrays
[10.3204/PUBDB-2023-03968]
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