Anisotropic Approach: Compact star as generalized Model
arXiv:2310.11842 · doi:10.1007/s10509-023-04171-9
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.
arXiv comment20 pages and 14 figures
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