Ушбу ишга иқтибос қилган ишлар

3 та иш

Иш: Can the dark energy equation-of-state parameter<i>w</i>be less than<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>−</mml:mi><mml:mn>1</mml:mn><mml:mi>?</mml:mi></mml:math>

1. Phantom black holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si302.svg" display="inline" id="d1e3235"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>,</mml:mo> <mml:mi>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity: From circular orbits to QPO tests

   Abubakir Shermatov, Javlon Rayimbaev, Sardor Murodov +5

   МақолаCosmology and Gravitation TheoriesPhysics of the Dark Universe20252 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.000983

2. Exact static and slowly rotating phantom conformal nonlinear-electrodynamic black holes in Bumblebee gravity with Lorentz Violation and shadow phenomenology

   Yassine Sekhmani, S. K. Maurya, Javlon Rayimbaev +3

   МақолаBlack Holes and Theoretical PhysicsPhysics of the Dark Universe20252 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.001163

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

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

   МақолаNoncommutative and Quantum Gravity TheoriesPhysics of the Dark Universe20250 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.001182