Regular quark star model with pressure anisotropy
Loading...
Date
2022
Authors
Journal Title
Journal ISSN
Volume Title
Publisher
Springer
Abstract
A new regular model for a stellar sphere with quark matter is found. The model satisfies a neutral quark star with pressure anisotropy. In this model, we consider an ansatz of a new form of one of the gravitational potentials, and stellar masses consistent with other findings which describe the generation of astrophysical objects. New masses, radii and surface gravitational red-shifts in acceptable ranges are also obtained using our model. The model satisfies stability and energy conditions. The state of hydrostatic equilibrium for stability is obtained by analysing the Tolman–Oppenheimer–Volkoff (TOV) equation. All other matter variables and gravitational potentials are well behaved.
Description
Abstract. Full text article available at https://doi.org/10.1007/s12043-022-02308-z
Keywords
Anisotropy, Neutral star, Quark matter, Stellar masses, Stability, Astrophysical objects, Quark star, Ansatz, Gravitational potentials
Citation
Mathias, A. V., & Sunzu, J. M. (2022). Regular quark star model with pressure anisotropy. Pramana, 96(2), 62.