  The main objective of this study is to investigate the phenomenon of the
bouncing scenario of the universe. The most widely recognized cosmological
framework is the standard cosmological model, sometimes referred to as the Big
Bang model. This is mainly because of its inherent properties and its
consistent alignment with recent observational studies. However, the standard
cosmological model faces some challenges concerning the physical conditions at
the initial epochs. Some of these issues include the initial singularity
problem, flatness problem, horizon problem, etc. Some of these challenges could
potentially be addressed by incorporating the inflationary scenario into the
cosmological framework of the universe. However, the inflationary mechanism is
not able to tackle the occurrence of the initial singularity. The bouncing
cosmology offers a probable solution to this initial singularity issue. In
addition, it is capable of addressing some other issues that may arise during
the early stages. Hence, in the modified gravity theory, bounce cosmology has
been discussed.
