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Modeling of non-rotating neutron stars in minimal dilatonic gravity

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arxiv 1608.06089 v2 pith:SOG35DII submitted 2016-08-22 gr-qc astro-ph.SR

Plamen Fiziev , Kalin Marinov This is my paper · ORCID
classification gr-qcastro-ph.SR
keywords modelbranse-dickedarkdilatoniceffectsequationsgravityminimal
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abstract

The model of minimal dilatonic gravity (MDG), called also the massive Branse-Dicke model with $\omega =0$, is an alternative model of gravitation, which uses one Branse-Dicke gravitation-dilaton field $\Phi$ and offers a simultaneous explanation of the effects of dark energy (DE) and dark matter (DM). Here we present an extensive research of non-rotating neutron star models in MDG with four different realistic equations of state (EOS), which are in agreement with the latest observational data. The equations describing static spherically symmetric stars in MDG are solved numerically. The effects corresponding to DE and DM are clearly seen and discussed.

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  1. White dwarfs in minimal dilatonic gravity

    gr-qc 2026-08 accept novelty 6.0 of 10

    White dwarfs in minimal dilatonic gravity are sub-Chandrasekhar for all scalar Compton lengths, with maximum mass dropping from 1.425 to 1.09 solar masses at λΦ = 500 km.

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