Manuel Malaver | Some new models for strange quark stars with isotropic pressure

ABSTRACT : We found new class of solutions to the Einstein-Maxwell system of equations for charged quark matter within the framework of MIT Bag Model considering a gravitational potential Z(x) proposed by Thirukkanesh and Ragel (2013), which depends on an adjustable parameter n. Variables as the energy density, charge density, pressure and the metric functions are written in terms of elementary and polinominal functions. We show that the form chosen for the gravitational potential allows obtain physically acceptable solutions with any value of the adjustable parameter.

ARXIV : 

https://arxiv.org/abs/1406.7347

  • Aucune note. Soyez le premier à attribuer une note !

Ajouter un commentaire

 

ENGLISH : EntropyFluid is the only complete scientific site written in both English and French! In the event of a bad translation, contact the administration via the "contact" tab.
FRENCH : EntropyFluid est le seul site scientifique complet rédigé à la fois en anglais et français !  En cas de mauvaise traduction, contactez l'administration via l'onglet "contact".