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Dilatonic Equation of Hydrostatic Equilibrium and Neutron Star Structure

In this paper, we present a new hydrostatic equilibrium equation related to dilaton gravity. We consider a spherical symmetric metric to obtain the hydrostatic equilibrium equation of stars in $4$-dimensions, and generalize TOV equation to the case of regarding a dilaton field. Then, we calculate the structure properties of neutron star using our obtained hydrostatic equilibrium equation employing the modern equations of state of neutron star matter derived from microscopic calculations. We show that the maximum mass of neutron star depends on the parameters of dilaton field and cosmological constant. In other words, by setting the parameters of new hydrostatic equilibrium equation, we calculate the maximum mass of neutron star.

preprint2015arXivOpen access
S. H. HendiG. H. BordbarB. Eslam PanahM. Najafi
astro-ph.HEgr-qchep-th
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S. H. HendiG. H. BordbarB. Eslam PanahM. Najafi

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