Anisotropic Compact Star with Vaidya-Tikekar Potential in $f(Q)$ Gravity

M. Awais; M. Azam

Anisotropic Compact Star with Vaidya-Tikekar Potential in $f(Q)$ Gravity

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2503.20792 v1 pith:5EUMYEFF submitted 2025-03-20 gr-qc

M. Awais , M. Azam This is my paper · ORCID

classification gr-qc

keywords modelphysicalsolutionanisotropicconstantsequationsgravityused

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

abstract

The goal of this work is to develop physical models for spherically symmetric systems in the realm of $f(Q)$ gravity. The field equations are set up for anisotropic fluid and formulate these equations using physical ansatz of Vaidya-Tikekar solution. The intrinsic constants of the model be ascertained by matching the interior solution to the external Schwarzschild solution. The use of accessibility conditions helps to understand the physical viability of the obtained model. LMC X-4 pulsar is used as a toy model to test the viability of the model and Mathematica software is used for deeper insights and visualization of the physical parameters against fixed values of constants.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Neutron stars in $f(\mathbb{Q})$ gravity
gr-qc 2025-12 conditional novelty 6.0 of 10

For f(Q)=Q+αQ² and f(Q)=Q^β, neutron-star solutions that admit power-series expansions at the center or at infinity collapse to General Relativity; genuine beyond-GR effects must be non-analytic.

Pith tools