← Назад к работе
Работы, цитирующие эту работу
Работ: 14
Работа: Constrained evolution of effective equation of state parameter in non-linear $\qquad\qquad f\left( {R,L_{m} } \right)$ dark energy model: insights from Bayesian analysis of cosmic chronometers and Pantheon samples
Exploring late-time cosmic acceleration: A study of a linear <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si6.svg" display="inline" id="d1e852"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> cosmological model using observational data
A. Zhadyranova, M. Koussour, S. Bekkhozhayev +2
ABIExploring 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
ABIExploring cosmological evolution and constraints in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si145.svg" display="inline" id="d1e758"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> teleparallel gravity
M. Koussour, Aziza Altaibayeva, S. Bekov +3
ABICosmological constraints on time-varying cosmological terms: A study of FLRW universe models with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si21.svg"><mml:mrow><mml:mi mathvariant="normal">Λ</mml:mi><mml:mo stretchy="true">(</mml:mo><mml:mi>t</mml:mi><mml:mo stretchy="true">)</mml:mo></mml:mrow></mml:math>CDM cosmology
M. Koussour, N. Myrzakulov, Javlon Rayimbaev
ABIConstraints on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si12.svg" display="inline" id="d1e927"><mml:mrow><mml:mi>Λ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>CDM cosmology using cosmic chronometers and supernova data
Yerlan Myrzakulov, M. Koussour, M. Bulanbay +2
ABI