Authors: Divyansh Mansukhani
While the ﬂatness problem, Ω = 1, has been one weighty stand in the modern cosmology to showcase incompetency of BBT, the theory of inﬂation - ﬁrst pioneered by Alan Guth, CTP, MIT (current) - serves to accommodate it in the observed universe. Here, (a) FP is used as a skeleton to attempt for an altogether novel approach involving rudimentary perturbation theory to deﬁne what one may call as ‘initial chaos’, and (b) the corresponding approach is postulated to be lightly rigorous than the other frameworks which propose in the same domain.
Comments: 2 Pages.
[v1] 2019-04-23 13:43:14
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