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6 та иш

Иш: The mass of the compact object in the X-ray binary her X-1/HZ her

  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

    МақолаCosmology and Gravitation TheoriesPhysics of the Dark Universe20242 иқтибос
    ABI

  2. Anisotropic compact stars under quintessence field with vanishing gravitational complexity factor

    S. Khan, Javlon Rayimbaev, Sarvar B. Iskandarov +3

    МақолаPulsars and Gravitational Waves ResearchPhysics of the Dark Universe20261 иқтибос
    ABI

  3. Nonlinear evolution of anisotropic matter configurations under higher-order curvature corrections

    A. Zahra, S. A. Mardan, Muhammad Bilal Riaz +4

    МақолаCosmology and Gravitation TheoriesThe European Physical Journal C20251 иқтибос
    ABI

  4. Modeling of Finch-Skea hybrid neutron stars with complexity-free characteristics

    S. Khan, Javlon Rayimbaev, Inomjon Ibragimov +3

    МақолаPulsars and Gravitational Waves ResearchPhysica Scripta20250 иқтибос
    ABI

  5. 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

    МақолаPulsars and Gravitational Waves ResearchPhysics of the Dark Universe20250 иқтибос
    ABI

  6. 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

    МақолаPulsars and Gravitational Waves ResearchAnnals of Physics20260 иқтибос
    ABI