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Иш: Bulk viscous matter in f(T) gravity: A path to cosmic acceleration
Constraints 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 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
ABICosmological inflation in<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>,</mml:mo><mml:mi mathvariant="script">G</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity
Mariafelicia De Laurentis, Mariacristina Paolella, Salvatore Capozzıello
Мақола20159 иқтибосABIModeling wormholes in <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>,</mml:mo><mml:mi>T</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity
P. H. R. S. Moraes, P. K. Sahoo
Мақола20178 иқтибосABILate-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 fits
Yerlan Myrzakulov, Orhan Dönmez, M. Koussour +3
ABIFitting <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4298" altimg="si614.svg"> <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 models with a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4315" altimg="si606.svg"> <mml:mi>Λ</mml:mi> </mml:math> CDM limit using <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e4320" altimg="si18.svg"> <mml:mrow> <mml:mi>H</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>z</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> and Pantheon data
José Antonio Nájera, Amanda Fajardo
Мақола20217 иқтибосABI