Axion Halo around a Binary System of Dwarf Stars
DOI:
https://doi.org/10.15407/ujpe69.7.472Keywords:
axion like particles, axion halo, dwarf starAbstract
The gravitational field of a clump of ultralight axion like particles (ALPs) in its core with a rotating binary system of dwarf stars is computed. It is established that the induced quadrupole mass moment of the clump is controlled parametrically by the Ma/M mass ratio of the axion clump and the binary core.
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