Nonthermal axion dark radiation and constraints

Mazumdar, Anupam and Qutub, Saleh and Saikawa, Ken'ichi (2016) Nonthermal axion dark radiation and constraints. Physical Review D, 94 (6). ISSN 1550-7998

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Abstract

The Peccei-Quinn mechanism presents a neat solution to the strong CPproblem. As a by-product, it provides an ideal dark matter candidate, “the axion”, albeit with a tiny mass. Axions therefore can act as dark radiation if excited with large momenta after the end of inflation. Nevertheless, the recent measurement of relativistic degrees of freedom from cosmic microwave background radiation strictly constrains the abundance of such extra relativistic species. We show that ultrarelativistic axions can be abundantly produced if the Peccei-Quinn field was initially displaced from the minimum of the potential. This in lieu places an interesting constraint on the axion dark matter window with large decay constant which is expected to be probed by future experiments. Moreover, an upper bound on the reheating temperature can be placed, which further constrains the thermal history of our Universe.

Item Type: Journal Article
Journal or Publication Title: Physical Review D
Additional Information: © 2016 American Physical Society
Departments: Faculty of Science and Technology > Physics
ID Code: 83214
Deposited By: ep_importer_pure
Deposited On: 28 Nov 2016 15:34
Refereed?: Yes
Published?: Published
Last Modified: 14 Oct 2019 08:37
URI: https://eprints.lancs.ac.uk/id/eprint/83214

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