The anisotropic component for examining dense objects like unfamiliar stars, compact objects, etc. has become different in Astrophysics. This chapter aims to resolve the physical management of some anisotropic compact star models in the back- ground of a core dark energy field. Next, we acquire the equatings of motion with the magnetic field of currents and modified Chaplygin vapor in f(T) gravity. Then corresponding conditions have been emphasize to discuss anisotropic management, stability of strength conditions, security analysis with adiabatic index, bulk, compactness, and surface redshift. It still observes the maximum energy mass and radial pressure principles for different compact stars. Finally, it is equated with the practical data in cases of differing types of compact stars.
Author(s) Details:
Pameli Saha,
Department
of Mathematics, Brainware University, Barasat, Kolkata-700125, India.
Ujjal
Debnath,
Department
of Mathematics, Indian Institute of Engineering Science and Technology,
Shibpur, Howrah-711103, India.
Please see the link here: https://stm.bookpi.org/CPPSR-V2/article/view/12047
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