Betelgeuse Constraints on Coupling between Axion-like Particles and Electrons
arXiv:2204.03121 · doi:10.1103/PhysRevD.106.123019
Abstract
Axion-like particles (ALPs) can be produced by thermal processes in a stellar interior, escape from the star and, if sufficiently light, be converted into photons in the external Galactic magnetic field. Such a process could produce a detectable hard X-ray excess in the direction of the star. In this scenario, a promising class of targets is the red supergiants, massive stars which are experiencing the late part of their evolution. We report on a search for ALP-induced X-ray emission from Betelgeuse, produced via the combined processes of Bremsstrahlung, Compton and Primakoff. Using a 50 ks observation of Betelgeuse by the \emph{NuSTAR} satellite telescope, we set 95\% C.L. upper limits on the ALP-electron () and ALP-photon () couplings. For masses eV, we find GeV (depending on the stellar model and assuming a value of the regular Galactic magnetic field in the direction transverse to Betelgeuse of =1.4 G). This corresponds to for GeV. This analysis supercedes by over an order of magnitude the limit on placed by the CAST solar axion experiment and is among the strongest constraints on these couplings.
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Cited by in corpus (7)
- Axion Astrophysics
- Investigation of the concurrent effects of ALP-photon and ALP-electron couplings in Collider and Beam Dump Searches
- Modeling of axion and electromagnetic fields coupling in a particle-in-cell code
- Probing the Axion-Nucleon Coupling with Supergiant Stars
- Searching for Axion-Like Particles with X-ray Observations of Alpha Centauri
- Search for Axion-Like Particles from Nearby Pre-Supernova Stars
- Axion-like particle constraints from preSN in future experiments