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Работы, на которые ссылается эта работа
Работ: 127
Работа: Parametrization of the deceleration parameter in a flat FLRW universe: constraints and comparative analysis with the $\Lambda $CDM paradigm
Cosmological tests of parametrization q = α − β H in f(Q) FLRW cosmology
Amine Bouali, B. K. Shukla, Himanshu Chaudhary +3
Статья2023Цитирований: 16ABICurrent constraints on the epoch of cosmic acceleration
B. Santos, J. Carvalho, J. S. Alcaniz
Статья2011Цитирований: 15ABIA divergence-free parametrization of deceleration parameter for scalar field dark energy
Статья2016Цитирований: 13ABITesting late-time cosmic acceleration with uncorrelated baryon acoustic oscillation dataset
David Benisty, Denitsa Staicova
Статья2020Цитирований: 12ABICosmic chronometers: constraining the equation of state of dark energy. I: H(z) measurements
Daniel Stern, Raul Jimenez, Licia Verde +2
Статья2010Цитирований: 12ABIThree thermodynamically based parametrizations of the deceleration parameter
Sérgio del Campo, Iván Mauricio Durán, Ramón Herrera +1
Статья2012Цитирований: 12ABITesting late-time cosmic acceleration with uncorrelated baryon acoustic oscillation dataset
David Benisty, Denitsa Staicova
Статья2021Цитирований: 11ABIProbing kinematics and fate of the Universe with linearly time-varying deceleration parameter
Özgür Akarsu, Tekin Dereli, Suresh Kumar +1
Статья2014Цитирований: 11ABIDo Type Ia Supernovae Provide Direct Evidence for Past Deceleration of the Universe?
Michael S. Turner, Adam G. Riess
Статья2002Цитирований: 11ABIBaryon acoustic oscillations in the Ly<i>α</i>forest of BOSS quasars
N. G. Busca, T. Delubac, J. Rich +59
Статья2013Цитирований: 10ABICosmological test of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si211.svg" display="inline" id="d1e1497"> <mml:mfrac> <mml:mrow> <mml:mi>σ</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>θ</mml:mi> </mml:mrow> </mml:mfrac> </mml:math> as function of scale factor in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.svg" display="inline" id="d1e1507"> <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> framework
Himanshu Chaudhary, Aditya Kaushik, Ankita Kohli
Статья2023Цитирований: 10ABI