Shamaila Rani

Энг кўп иқтибос қилинган асарлар

1. Thermodynamic properties and geometries of bardeen black hole surrounded by string clouds20243 иқтибос
2. 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 solutions20242 иқтибос
3. Cosmic and thermodynamics consequences of Chaplygin–Jacobi corrected HDE model20251 иқтибос
4. Cosmic analysis through dark energy models in fractal universe with non-linear interaction term20240 иқтибос
5. Stability and topological thermodynamics of black holes through modified entropy20250 иқтибос
6. Constraining Big Bang nucleosynthesis in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"> <mml:mi>f</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:mi>T</mml:mi> <mml:mo>,</mml:mo> <mml:mi>B</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>T</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="script">G</mml:mi> </mml:mrow> </mml:msub> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>B</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="script">G</mml:mi> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> </mml:math> gravity20250 иқтибос
7. Probing thermodynamics of Einstein–Maxwell scalar black hole through exponential corrected entropy20250 иқтибос
8. Observational constraining on inflationary parameters in Barrow inspired f(R) cosmology20250 иқтибос
9. Thermodynamics analysis of black hole through modified entropies by applying Hawking evaporation phenomenon20260 иқтибос
10. Chaos bounds or violation? Fate of charged AdS black holes20260 иқтибос