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Иш: Model-independent parameterization of H(z) and its implications for cosmic evolution
Large scale structure as a probe of gravitational slip
Scott F. Daniel, Robert R. Caldwell, Asantha Cooray +1
Мақола200817 иқтибосABIConstraints on the redshift dependence of the dark energy potential
Joan Simón, Licia Verde, Raúl Jiménez
Мақола200515 иқтибосABIA new Om(z) diagnostic of dark energy in general relativity theory
N. Myrzakulov, M. Koussour, Dhruba Jyoti Gogoi
Мақола202315 иқтибосABIInvestigating the dark energy phenomenon in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si14.svg" display="inline" id="d1e553"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>R</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> cosmological models with observational constraints
S. Myrzakulova, M. Koussour, N. Myrzakulov
Мақола202313 иқтибосABIConstraints on bulk viscosity in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si256.svg" display="inline" id="d1e1685"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity from H(z)/Pantheon+ data
M. Koussour, Abdelghani Errehymy, Orhan Dönmez +4
Мақола202413 иқтибосABIExploring accelerated expansion in the universe: A study of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si274.svg" display="inline" id="d1e325"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity with parameterized EoS and cosmological constraints
M. Koussour, N. Myrzakulov, Javlon Rayimbaev +2
ABIObservational constraints on the equation of state of viscous fluid in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si250.svg" display="inline" id="d1e314"><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
M. Koussour, Aziza Altaibayeva, S. Bekov +3
ABIIs there supernova evidence for dark energy metamorphosis?
Ujjaini Alam, Varun Sahni, Tarun Deep Saini +1
Мақола20048 иқтибосABIReconciling dark energy models with<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>theories
Salvatore Capozzıello, V. F. Cardone, A. Troisi
Мақола20058 иқтибосABI