Axion stars in MGD background

The minimal geometric deformation (MGD) paradigm is here employed to survey axion stars on fluid branes. finite value of the brane tension provides beyond-general relativity corrections density, compactness, radius, and asymptotic limit gravitational mass function stars, in a MGD background. also enhances effective range magnitude field coupled gravity. are compatible mini-massive compact halo objects for almost all observational tension, however, narrow allows star densities large enough produce stimulated decays photons, with no analogy general-relativistic (GR) limit. Besides, density shown be up four orders larger than GR being less sensitive tidal disruption events under collision neutron lower values tension.