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5 ta ish

Ish: Causal limit of neutron star maximum mass in f(R) gravity in view of GW190814

  1. A Brief analysis of isotropic Karmarkar models in modified gravity theory

    Yihu Feng, Tayyab Naseer, Asifa Ashraf +2

    MaqolaCosmology and Gravitation TheoriesChinese Journal of Physics20248 iqtibos
    ABI

  2. Electrically charged black holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si6.svg" display="inline" id="d1e1021"><mml:mrow><mml:mi>F</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>-Euler–Heisenberg theory

    Yassine Sekhmani, S. K. Maurya, M. K. Jasim +2

    MaqolaCosmology and Gravitation TheoriesPhysics of the Dark Universe20242 iqtibos
    ABI

  3. Non-singular anisotropic hybrid star model in f(ℛ,𝒜) theory of gravity

    Adnan Malik, Amjad Hussain, Shahid Chaudhary +4

    MaqolaGeophysics and Gravity MeasurementsInternational Journal of Geometric Methods in Modern Physics20252 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. Charged Spherical Solution in Torsion and Matter Coupling Gravity and Influence of Torsion Parameter and Electric Charge on Compact Stars in Lower Mass Gap

    S. K. Maurya, Abdelghani Errehymy, Ghulam Mustafa +3

    MaqolaOchiq kirishGeophysics and Gravity MeasurementsProgress of Theoretical and Experimental Physics20240 iqtibos
    ABI