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Ish: Influence of pressure anisotropy on mass-radius relation and stability of millisecond pulsars in f(Q) gravity

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   ABIABI:AkademIndex/openalex/2026.other.109622

2. Role of three coupling parameters on maximum mass and stability: Theoretical insights into relativistic massive compact objects in mass gap under <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si334.svg" display="inline" id="d1e10703"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> action

   S. K. Maurya, Abdelghani Errehymy, Y. Saginayev +4

   MaqolaCosmology and Gravitation TheoriesPhysics of the Dark Universe20251 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000793