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arxiv: 1305.1087 · v2 · pith:XZMUYNZYnew · submitted 2013-05-06 · 🌌 astro-ph.SR · gr-qc

Chameleon dark matter stars

Vladimir Folomeev , Ascar Aringazin , Vladimir Dzhunushaliev This is my paper
classification 🌌 astro-ph.SR gr-qc
keywords darkmatterfieldchameleonconfigurationscouplingformscalar
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We consider static, spherically symmetric equilibrium configurations consisting of fermionic dark matter nonminimally coupled to dark energy in the form of a quintessence scalar field. With the scalar field coupling function, the form of which is taken to meet cosmological observations, we estimate the effect of such a nonminimal coupling on the properties of dark matter compact configurations. We show that the masses and sizes of the resulting chameleon dark matter stars are smaller than those of systems with no field present.

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  1. Scalarization of dark matter stars

    gr-qc 2026-05 unverdicted novelty 5.0

    Scalarization occurs across most of the parameter space for negative coupling parameter β_d in self-interacting dark matter stars, over a broader range than in conventional neutron stars.