https://doi.org/10.1140/epjc/s10052-024-13369-2
Regular Article - Theoretical Physics
Anisotropic model observing pulsars from Neutron Star Interior Composition with modified Van der Waals equation of state
1
Department of Mathematics, University of Management and Technology, Lahore, Pakistan
2
IT4Innovations, VSB-Technical University of Ostrava, Ostrava, Czech Republic
3
Department of Computer Science and Mathematics, Lebanese American University, Byblos, Lebanon
a ayeshakhalid4238@gmail.com, S2019109012@umt.edu.pk
Received:
22
August
2024
Accepted:
15
September
2024
Published online:
8
October
2024
This paper is designed for heavy pulsars coming from the Neutron Star Interior Composition Explorer. The research model is describe by Einstein field equations for anisotropic fluid configuration with spherical symmetry. As per present perceptiveness, modified non-linear Van der Waals equation of state is used to relate physical variables. The continuity of inner and outer matter is obtained by comparing inner spacetime to outer Schwarzschild metric. The physical viability of this model is evaluated and further it is compared with observational data of pulsars PSR J0348+0432, PSR J0740+6620 and PSR J0030+0451. The model fulfils all physical and mathematical characteristics of the dense structure studies. It offers the factual proofs carried by evolution of celestial configurations. The working model presented here is physically viable and shows stable behaviour.
© The Author(s) 2024
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Funded by SCOAP3.
