Isocurvature bounds on axion-like particle dark matter in the post-inflationary scenario
We assume that dark matter is comprised of axion-like particles (ALPs) generated by the realignment mechanism in the post-inflationary scenario. This leads to isocurvature fluctuations with an amplitude of order one for scales comparable to the horizon at the time when the ALP field starts oscillati...
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| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
14 May 2019
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| In: |
Journal of cosmology and astroparticle physics
Year: 2019, Heft: 5 |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2019/05/021 |
| Online-Zugang: | Verlag, Pay-per-use, Volltext: https://doi.org/10.1088/1475-7516/2019/05/021
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| Verfasserangaben: | M. Feix, J. Frank, A. Pargner, R. Reischke, B.M. Schäfer and T. Schwetz |
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| 520 | |a We assume that dark matter is comprised of axion-like particles (ALPs) generated by the realignment mechanism in the post-inflationary scenario. This leads to isocurvature fluctuations with an amplitude of order one for scales comparable to the horizon at the time when the ALP field starts oscillating. The power spectrum of these fluctuations is flat for small wave numbers, extending to scales relevant for cosmological observables. Denoting the relative isocurvature amplitude at k* = 0.05 Mpc−1 by fiso, Planck observations of the cosmic microwave background (CMB) yield fiso < 0.31 at the 2σ-level. This excludes the hypothesis of post-inflationary ALP dark matter with masses ma < 10−20-10−16 eV, where the range is due to details of the ALP mass-temperature dependence. Future CMB stage IV and 21-cm intensity mapping experiments may improve these limits by 1-2 orders of magnitude in ma. | ||
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