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Ish: Dehnen-type dark matter wormholes in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg" display="inline" id="d1e414"> <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> action

  1. Physical viability of the general relativistic wormholes sourced by dark matter distributions

    Z. Yousaf, Mohammad Alshammari, M. Rizwan +3

    MaqolaDark Matter and Cosmic PhenomenaPhysics of the Dark Universe20260 iqtibos
    ABI

  2. Light trajectories and shadows of slowly rotating wormholes in void environments

    Abdelghani Errehymy, M. Govender, O. Donmez +3

    MaqolaFluid Dynamics and Thin FilmsPhysics Letters B20260 iqtibos
    ABI

  3. 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

  4. Holographic dark energy as a source for slowly rotating wormholes: Implications for null geodesics and shadows

    Abdelghani Errehymy, S. K. Maurya, M. Govender +4

    MaqolaCosmology and Gravitation TheoriesPhysics Letters B20260 iqtibos
    ABI