Modeling compact stellar objects admitting anisotropic fluid in f ( R , T ) gravity: Viability and stability analysis
Key Points
Compact stellar objects exhibit distinct stability characteristics under anisotropic fluid conditions, suggesting complex behaviors in gravity.
The analysis employs mathematical modeling to assess the viability of these objects, revealing their structural integrity under different gravitational scenarios.
Employing advanced mathematical techniques, the research explores stability factors that influence the formation of compact stellar objects in gravitational fields.
Findings present significant implications for understanding gravity's role in stellar formations, requiring further exploration in astrophysical contexts.