Abstract
The effect of a magnetized plasma on the resonant photoproduction of axions on the electromagnetic multipole components of the medium, i → f + a, has been considered. It has been shown that the axion emissivity in the resonance region, owing to various reactions involving particles of the medium, is certainly expressed in terms of the emissivity of the photon → axion transition. The number of axions produced by the equilibrium cosmic microwave background radiation in the magnetar magnetosphere has been determined. It has been shown that the resonant mechanism under consideration is inefficient for the production of cold dark mass.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
