Analysis of cosmological parameters in a gravity model explains accelerated expansion, suggesting a link to current observations.
According to a number of astronomical studies, the universe is currently undergoing an accelerated expansion phase. We employed the recently proposed gravity, which holds that the current accelerated expansion phase of the universe is caused by a torsion scalar. The investigation is carried out using a parameterization of [Formula: see text] (where [Formula: see text] and [Formula: see text] are the model parameters) and the [Formula: see text] using [Formula: see text] is obtained. The model shows good agreement with recent observations, such as the LCDM model at late times. Finally, we examined how the cosmological parameters behaved in for constrained values.
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Shekh et al. (2024) studied this question.
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