# LRS Bianchi type-I cosmological model with constant deceleration parameter in $f(R,T)$ gravity

Source: [LRS Bianchi type-I cosmological model with constant deceleration parameter in $f(R,T)$ gravity](<https://www.sota2.com/research/paper/68fa42171e209131ce8ff929>)

Collection index: [llms.txt](<https://www.sota2.com/research/llms.txt>)

Data updated: 2025-10-25T03:37:08.074Z

Authors: Binaya K. Bishi, S.K.J. Pacif, P.K. Sahoo, G.P. Singh

Published: 2017-06-23T18:14:27.000Z

## Abstract

A spatially homogeneous anisotropic LRS Bianchi type-I cosmological model is studied in $f(R,T)$ gravity with a special form of Hubble's parameter, which leads to constant deceleration parameter. The parameters involved in the considered form of Hubble parameter can be tuned to match, our models with the $\\Lambda $CDM model. With the present observed value of the deceleration parameter, we have discussed physical and kinematical properties of a specific model. Moreover, we have discussed the cosmological distances for our model.

## Recorded benchmark results

A research result applies to its stated dataset, split, metric and evaluation configuration. Compare like-for-like settings, preserve the metric's unit and direction, and distinguish paper-reported results from independent reproduction. The best result recorded here is not a claim of exhaustive, current global coverage.

## Original sources and implementation

[Original paper](<https://arxiv.org/abs/1706.08844>)

[PDF](<https://arxiv.org/pdf/1706.08844.pdf>)