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6 та иш

Иш: Gravitational waves at the first post-Newtonian order with the Weyssenhoff fluid in Einstein–Cartan theory

  1. Einasto-inspired non-commutative black holes within dark matter galactic halos in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si8.svg" display="inline" id="d1e849"><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

    S. Khan, Javlon Rayimbaev, Inomjon Ibragimov +2

    МақолаBlack Holes and Theoretical PhysicsAnnals of Physics20254 иқтибос
    ABI

  2. Gravitationally decoupled anisotropic compact stars immersed in Dehnen-(1,4,0) density profiles

    S. Khan, Javlon Rayimbaev, Otaboyev Sirajiddin +3

    МақолаDark Matter and Cosmic PhenomenaNuclear Physics B20262 иқтибос
    ABI

  3. 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

  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. Electromagnetic field and anisotropic minimally complex quintessence stars

    S. Khan, Javlon Rayimbaev, Munisbek Akhmedov +3

    МақолаPulsars and Gravitational Waves ResearchModern Physics Letters A20260 иқтибос
    ABI

  6. Torsionally corrected anisotropic spherical halos via gravitational decoupling in a dark matter medium

    S. Khan, Javlon Rayimbaev, Jakhongir Kurbanov +2

    МақолаDark Matter and Cosmic PhenomenaPhysics of the Dark Universe20260 иқтибос
    ABI