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4 ta ish

Ish: On the stability and physical properties of an exact relativistic model for a superdense star

  1. 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

    MaqolaGeophysics and Gravity MeasurementsProgress of Theoretical and Experimental Physics20240 iqtibos
    ABI

  2. Testing linear non-minimal coupling in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si447.svg" display="inline" id="d1e4384"> <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> gravity using X-ray binary pulsars constrained by NICER observations

    Abdelghani Errehymy, S. K. Maurya, Orhan Dönmez +4

    MaqolaPulsars and Gravitational Waves ResearchPhysics of the Dark Universe20250 iqtibos
    ABI

  3. Self-consistent and stable stellar structures in massive gravity

    M. R. Shahzad, Wajiha Habib, Asifa Ashraf +3

    MaqolaCosmology and Gravitation TheoriesPhysics of the Dark Universe20250 iqtibos
    ABI

  4. Constraining <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si170.svg" display="inline" id="d1e5067"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi mathvariant="script">L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity with NICER/NuSTAR observations of X-ray Pulsars

    S. K. Maurya, Abdelghani Errehymy, Orhan Dönmez +4

    MaqolaPulsars and Gravitational Waves ResearchAnnals of Physics20260 iqtibos
    ABI