# A realistic model of a neutron star in minimal dilatonic gravity

@article{Fiziev2015ARM, title={A realistic model of a neutron star in minimal dilatonic gravity}, author={Plamen P. Fiziev}, journal={arXiv: General Relativity and Quantum Cosmology}, year={2015} }

We present a derivation of the basic equations and boundary conditions for relativistic static spherically symmetric stars (SSSS) in the model of minimal dilatonic gravity (MDG) which offers an alternative and simultaneous description of the effects of dark matter (DM) and dark energy (DE) using one dilaton field $\Phi$. The numerical results for a realistic equation of state (EOS) MPA1 of neutron matter are presented for the first time. The three very different scales, the Compton length of…

## 3 Citations

Towards New Constraints in Extended Theories of Gravity: Cosmography and Gravitational-Wave Signals from Neutron Stars

- Physics
- 2018

Combined cosmological, astrophysical and numerical tests may shed some light on the viability of theories of gravity beyond Einsteinian relativity. In this letter, we present two different techniques…

Compact static stars in minimal dilatonic gravity

- Physics
- 2017

In the version1 of this paper we presented for the first time the basic equations and relations for relativistic static spherically symmetric stars (SSSS) in the model of minimal dilatonic gravity…

The mass of dark scalar and phase space analysis of realistic models of static spherically symmetric objects

- Mathematics
- 2015

We consider singularities of static spherically symmetric objects in minimal dilatonic gravity. They are only partially studied and purely understood even in the simplest models of extended gravity.…

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