Перейти к основному содержанию
AkademIndex

Продукты

Для разработчиков

AkademBaseОткрытый API экосистемы
← Назад к работе

Работы, цитирующие эту работу

Работ: 6

Работа: 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

    СтатьяCosmology and Gravitation TheoriesPhysics of the Dark Universe2024Цитирований: 2
    ABI

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

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

    СтатьяPulsars and Gravitational Waves ResearchPhysics of the Dark Universe2026Цитирований: 1
    ABI

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

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

    СтатьяCosmology and Gravitation TheoriesThe European Physical Journal C2025Цитирований: 1
    ABI

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

    S. Khan, Javlon Rayimbaev, Inomjon Ibragimov +3

    СтатьяPulsars and Gravitational Waves ResearchPhysica Scripta2025Цитирований: 0
    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

    СтатьяPulsars and Gravitational Waves ResearchPhysics of the Dark Universe2025Цитирований: 0
    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

    СтатьяPulsars and Gravitational Waves ResearchAnnals of Physics2026Цитирований: 0
    ABI