Anisotropic Approach: Compact star as generalized Model

Abstract

We studied a new class of interior solutions that are singular-free and useful for describing anisotropic compact star objects with spherically symmetric matter distribution. We have considered metric potential selecting B_0^2 (r)=1/(1-r^2/R^2 )^n ,where n>2 . The various physical characteristics of the model are specifically examined for the pulsar PSRJ1903+327 with its current estimated data. According to analysis, every physical need for a physically admissible star is satisfied and all features are acceptable. Further, the stability of the model has been examined. Numerous physical characteristics are also highlighted in a graphical form.

20 pages and 14 figures

References in corpus (10)

• Sound Speeds, Cracking and Stability of Self-Gravitating Anisotropic Compact Objects
• A class of relativistic stars with a linear equation of state
• Anisotropic models for compact stars
• Charged anisotropic models for quark stars
• Analytical models for quark stars
• Singularity free anisotropic strange quintessence star
• Modified Finch and Skea stellar model compatible with observational data
• The Dark Energy Star and Stability analysis
• Finch-Skea star model in f(R, T ) theory of gravity
• Anisotropic extension of Finch and Skea stellar model