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• W4307300871 abstract "The observational evidence regarding the present cosmological aspects tells us about the presence of very little anisotropy in the universe on a large scale. Here, in this paper, we attempt to study locally rotationally symmetric (LRS) homogeneous Bianchi-I spacetime with the isotropic matter distribution. This is done within the framework of f(R,ℒm) gravity. Particularly, we consider a non-linear f(R,ℒm) model, f(R,ℒm)=12R+ℒmα. Furthermore, ω, the equation of state parameter, which is vital stuff in determining the present phase of the universe is constrained. To constrain the model parameters and the equation of state parameter, we use 57 Hubble data points and 1048 Pantheon supernovae type Ia data sample. And, for our statistical analysis, we use Markov Chain Monte Carlo (MCMC) simulation. Moreover, with the help of obtained values of parameters, we measure the anisotropy parameter for our model." @default.
• W4307300871 created "2022-10-31" @default.
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• W4307300871 date "2022-12-01" @default.
• W4307300871 modified "2023-10-16" @default.
• W4307300871 title "Constraining anisotropic cosmological model in <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline id=d1e682 altimg=si6.svg><mml:mrow><mml:mi mathvariant=script class=mathpzc>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant=script>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> Gravity" @default.
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• W4307300871 doi "https://doi.org/10.1016/j.dark.2022.101126" @default.
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