id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
cana-5883	Vandana Soni, Sudha Agrawal	Bianchi Type V Universe with QVDP in f (R, T) Theory of Gravity	2025	15	.pdf	application/pdf	5042	297	62	In this paper, we have evolved anisotropic cosmological model in f(𝑅, 𝑇) gravity theory to acquire the exact solution of the alter field equations in the activity of the newly offered condition of [36] quadratic form of deceleration parameter and requiring the functional form of f(𝑅, 𝑇) = f1(R) + f2(T), where f1(R) = 𝜆 𝑅 and f2(T) = 𝜆 𝑇. The Hubble Parameter in the terms of redshift (z) conceivably expressed as, H = Ho [1± 1+𝑧 √𝑧(𝑧+2)+2 ] 3 −6𝛽[1± 1+𝑧 √𝑧(𝑧+2)+2 ] 2 +8 𝛽2[1± 1+𝑧 √𝑧(𝑧+2)+2 ] concerning red shift, Deceleration parameter can be stated as, q (z) = 𝑧2+2𝑧−1 𝑧2+2𝑧+2 (40)	cache/cana-5883.pdf	txt/cana-5883.txt