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Constraints on axions and axionlike particles from Fermi Large Area Telescope observations of neutron stars
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).
Number of Authors: 3
2016 (English)In: Physical Review D, ISSN 2470-0010, Vol. 93, no 4, 045019Article in journal (Refereed) Published
Abstract [en]

We present constraints on the nature of axions and axionlike particles (ALPs) by analyzing gamma-ray data from neutron stars using the Fermi Large Area Telescope. In addition to axions solving the strong CP problem of particle physics, axions and ALPs are also possible dark matter candidates. We investigate axions and ALPs produced by nucleon-nucleon bremsstrahlung within neutron stars. We derive a phenomenological model for the gamma-ray spectrum arising from subsequent axion decays. By analyzing five years of gamma-ray data (between 60 and 200 MeV) for a sample of four nearby neutron stars, we do not find evidence for an axion or ALP signal; thus we obtain a combined 95% confidence level upper limit on the axion mass of 7.9 x 10(-2) eV, which corresponds to a lower limit for the Peccei-Quinn scale fa of 7.6 x 10(7) GeV. Our constraints are more stringent than previous results probing the same physical process, and are competitive with results probing axions and ALPs by different mechanisms.

Place, publisher, year, edition, pages
2016. Vol. 93, no 4, 045019
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-128179DOI: 10.1103/PhysRevD.93.045019ISI: 000370247600020OAI: oai:DiVA.org:su-128179DiVA: diva2:914140
Available from: 2016-03-23 Created: 2016-03-21 Last updated: 2016-03-23Bibliographically approved

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Meyer, Manuel
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