Study of Cosmological Aspects in Chern-Simons Modified Gravity

Abstract

We offer a cosmological model where the cosmos recovers in an non-unique recovery. Following the bounce, it slows down in some cases, the main evolu- tion is similar to matter The era of deceleration, and finally the current era, is evolving through a phase of acceleration. Our goal is to investigate this behav- ior using the modified F (R) gravity, Chern-Simons theory, and to compare the concept to other empirical evidence. We calculate the shape of the entire F(R) conceivable cosmic time horizon using enabled the development and the rele- vant process parameters. The quasi jump appears to be associated with periods of DE, particularly from quasi bounces to slowdowns as well as from the re- tardation era to the late acceleration era, according to the structure of F(R). It is vital to recognize that the script’s rebound in this situation is an uneven bounce, particularly because the Hubble radius is monotonic. It gradually increases and gradually differentiates in the latter part of ca, while it seems to decrease grad- ually over time now. Decreasing behavior of Hubble beam ensures delayed acceleration cosmic age. Furthermore, due to the aforementioned the Hubble radius’s development, prototype disturbance patterns occur during deep con- tractions away from rebounds, when all the perturbation function is coming. We calculate gradient and tensile strength separately spectral, so we evaluate raw observations such as spectral metrics gradient curvature misalignment, stretch- ing the gradient ratio, therefore, in I agree with the most recent Planck 2018 limitations. The term CS¢aappears to, in this meaning, it has a significant effect on the development of tensor barriers, but keeps the gradient part constant, the perturbation in the case of the vacuum model F(R), therefore, CS the term seems to play an vital role in reconciling observable with Planck result.