Yerlan Myrzakulov

Энг кўп иқтибос қилинган асарлар

1. Linear redshift parametrization of deceleration parameter in f(R,Lm) gravity202410 иқтибос
2. 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 viscosity20259 иқтибос
3. Late-time cosmology in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si23.svg" display="inline" id="d1e469"><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: Analytical solutions and observational fits20247 иқтибос
4. Model-independent parameterization of H(z) and its implications for cosmic evolution20247 иқтибос
5. Probing the universe's expansion dynamics: The linear correction scenario perspective on dark energy20243 иқтибос
6. Signature flips in time-varying $$\Lambda (t)$$ cosmological models with observational data20243 иқтибос
7. Energy conditions in $$f(Q, L_m)$$ gravity20251 иқтибос
8. Thermodynamic constraints and observational validation of the deceleration parameter20251 иқтибос
9. Non-singular bouncing cosmology in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si16.svg" display="inline" id="d1e237"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>T</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="script">T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity with energy condition violations20251 иқтибос
10. Event horizon telescope observational constraints on Dymnikova-type non-singular black holes in higher dimensions20261 иқтибос