The arions generation by magnetodipole waves of pulsars and magnetars in a constant magnetic field
V.I. Denisov, G.A. Dantsev, V.I. Priclonsky, I.P. Denisova, O.N., Gavrish

TL;DR
This paper evaluates how gravitational fields of pulsars and magnetars influence arion emission during magnetodipole wave propagation in a constant magnetic field, deriving flux, amplitude, and energy growth characteristics.
Contribution
It provides a new analytical solution for arion flux and energy growth in a constant magnetic field influenced by pulsars and magnetars, including an estimate of the photon-arion coupling constant.
Findings
Arion wave amplitude tends to a constant at large distances.
Arion emission energy grows quadratically with distance in a constant magnetic field.
The results are applicable within a finite coherence length where magnetic field lines are straight.
Abstract
The influence of the gravitational fields of pulsars and magnetars on the arion emission during the propagation of magnetodipole waves in a constant magnetic field has been evaluated. The solution of the equation was obtained and the flux of arions emitted by magnetodipole waves during their propagation in a constant magnetic field was found. It is shown that the amplitude of the born arion wave at a distance from the source of magnetodipole radiation of a pulsar or magnetar in the considered case tends to a constant value. The intensity of the arion emission in the solid angle element and the amount of arion energy , emitted in all directions per unit time grow quadratically with increasing distance, traveled by the magnetodipole radiation of a pulsar or magnetar in a constant magnetic field. Such growth of the energy of the born arion wave is due to…
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Taxonomy
TopicsMagnetic Properties of Alloys · Solid-state spectroscopy and crystallography · Electromagnetic Effects on Materials
