Charged anisotropic models for quark stars
arXiv:1412.8140 · doi:10.1007/s10509-014-1918-7
Abstract
We perform a detailed physical analysis for a class of exact solutions for the Einstein-Maxwell equations. The linear equation of state consistent with quark stars has been incorporated in the model. The physical analysis of the exact solutions is performed by considering the charged anisotropic stars for the particular nonsingular exact model obtained by Maharaj, Sunzu and Ray. In performing such an analysis we regain masses obtained by previous researchers for isotropic and anisotropic matter. It is also indicated that other masses and radii may be generated which are in acceptable ranges consistent with observed values of stellar objects. A study of the mass-radius relation indicates the effect of the electromagnetic field and anisotropy on the mass of the relativistic star.
11 pages, Submitted for publication
References in corpus (10)
- Charged anisotropic matter with linear equation of state
- A class of relativistic stars with a linear equation of state
- Electrically Charged Strange Quark Stars
- Classes of exact Einstein-Maxwell solutions
- The role of pressure anisotropy on the maximum mass of cold compact stars
- Analytical models for quark stars
- Tikekar superdense stars in electric fields
- A Polytropic Model of Quark Stars
- Charged relativistic spheres with generalized potentials
- Generalised compact spheres in electric fields
Cited by in corpus (11)
- Quark star model with charged anisotropic matter
- Modified Finch and Skea stellar model compatible with observational data
- A family of Finch and Skea relativistic stars
- Effects of Gravity on Anisotropic Charged Compact Structures
- Charged Anisotropic Models with Complexity-free Condition
- Anisotropic extension of Finch and Skea stellar model
- New charged anisotropic compact models
- Charged Anisotropic Tolman IV Solution in Matter-Geometry Coupled Theory
- Relativistic structure of charged quark stars in energy-momentum squared gravity
- Compact stellar model in presence of pressure anisotropy in modified Finch Skea spacetime
- Anisotropic Approach: Compact star as generalized Model