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Ish: Inhomogeneous equation of state of the universe: Phantom era, future singularity, and crossing the phantom barrier

1. Constraining <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si140.svg" display="inline" id="d1e319"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>Q</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity with bulk viscosity

   Yerlan Myrzakulov, Orhan Dönmez, M. Koussour +3

   MaqolaCosmology and Gravitation TheoriesPhysics of the Dark Universe20259 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000038

2. Kalb-Ramond black holes sourced by ModMax electrodynamics: Some perturbative properties in the phantom sector

   Yassine Sekhmani, Anshuman Baruah, S. K. Maurya +4

   MaqolaNoncommutative and Quantum Gravity TheoriesPhysics of the Dark Universe20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.001182

3. Black holes surrounded by a Murnaghan-fluid scalar gas in a global-monopole background

   Yassine Sekhmani, S. K. Maurya, Javlon Rayimbaev +4

   MaqolaAstrophysical Phenomena and ObservationsPhysics of the Dark Universe20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.010544