A physics hypothesis called the Big Bang event explains how the cosmos grew from a highly dense and hot starting condition. The evolution of the observable universe from the earliest known times to its succeeding large-scale shape is explained by several cosmological theories of the Big Bang. A wide range of observable phenomena, such as the quantity of light elements, the cosmic microwave background (CMB) radiation, and large-scale structure, are all thoroughly explained by these theories. Cosmic inflation, or the abrupt and extremely fast expansion of space during the Universe's early moments, provides an explanation for the uniformity of the Universe as a whole, sometimes known as the "flatness issue." Yet there isn't yet a generally recognised quantum gravity theory in physics that can accurately simulate the Big Bang's early circumstances. Precise studies of the universe's expansion rate establish the Big Bang singularity at an estimated 13.7870.020 ...