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5 ta ish

Ish: On the nature and evolution of the unique binary pulsar J1903+0327

  1. Physical viability of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.svg" display="inline" id="d1e120"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="double-struck">Q</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity corrected charged anisotropic solutions

    Shamaila Rani, Muhammad Adeel, M. Zeeshan Gul +2

    MaqolaCosmology and Gravitation TheoriesPhysics of the Dark Universe20247 iqtibos
    ABI

  2. Compact stellar objects beyond non-Riemannian geometry: A comprehensive study in f(Q, Lm, T) theory

    Aisha Siddiqa, M. Zeeshan Gul, Sadia Zahid +3

    MaqolaStellar, planetary, and galactic studiesPhysics of the Dark Universe20264 iqtibos
    ABI

  3. Exploring physical properties of spherically symmetric anisotropic stellar models with string clouds and quintessence field

    G. Mustafa, S. K. Maurya, Ibrar Hussain +3

    MaqolaCosmology and Gravitation TheoriesInternational Journal of Geometric Methods in Modern Physics20251 iqtibos
    ABI

  4. Constraining <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mi mathvariant="script">L</mml:mi> <mml:mi>m</mml:mi> </mml:msub> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:math> gravity with millisecond pulsar observations

    S.K. Maurya, A. Errehymy, K.N. Singh +4

    MaqolaOchiq kirish20261 iqtibos
    ABI

  5. Anisotropic compact stars in quadratic f(R) gravity and influence of quadratic parameter on properties of compact stars

    Rajesh Kumar, S. K. Maurya, Yassine Sekhmani +2

    MaqolaOchiq kirish20251 iqtibos
    ABI