Dark Energy and Dark Matter in Stars Physic
Abstract
We present the basic equations and relations for the relativistic static spherically symmetric stars (SSSS) in the model of minimal dilatonic gravity (MDG) which is {\em locally} equivalent to the f(R) theories of gravity and gives an alternative description of the effects of dark matter and dark energy. The results for the simplest form of the relativistic equation of state (EOS) of neutron matter are represented. Our approach overcomes the well-known difficulties of the physics of SSSS in the f(R) theories of gravity introducing two novel EOS for cosmological energy-pressure densities and dilaton energy-pressure densities, as well as proper boundary conditions.
Keywords
Cite
@article{arxiv.1411.0242,
title = {Dark Energy and Dark Matter in Stars Physic},
author = {Plamen Fiziev},
journal= {arXiv preprint arXiv:1411.0242},
year = {2014}
}
Comments
Latex file, 7 pages, 11 figures. Symposium "Frontiers of Fundamental Physics 14", Marseille, France. arXiv admin note: substantial text overlap with arXiv:1402.2813