id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
cana-5017	Swapnil S. Charjan	LRS Bianchi Type-I Magnetized Dark Energy Cosmological Model in Bimetric Theory of Relativity with Cosmological Term – Λ	2024	11	.pdf	application/pdf	4155	239	61	Solution of Field Equations Without Magnetic Field Case I: 𝜌 + 𝜆 = 0 When the magnetic field is not present equation (19) becomes 𝑑𝑠2 = − 𝑑𝑇2 [ 4𝛼 (4−𝑛)(𝑛+2)𝑇𝑛+𝑀𝑇2] + 𝑇2𝑛𝑑𝑋2 + 𝑇2(𝑑𝑌2 + 𝑑𝑍2) (36) Case II: 𝜌 − 𝜆 = 0 When the magnetic field is not present equation (25) becomes Communications on Applied Nonlinear Analysis ISSN: Through the proper coordinate transformation 𝐵 = 𝑇 , 𝑥 = 𝑋 , 𝑦 = 𝑌 𝑎𝑛𝑑 𝑧 = 𝑍 metric (4) becomes 𝑑𝑠2 = − 𝑑𝑇2 [ 96𝜋𝛫𝑇𝑛 (4−𝑛)(𝑛−2) + 4𝛼 (4−𝑛)(𝑛+2)𝑇𝑛+𝑀𝑇2] + 𝑇2𝑛𝑑𝑋2 + 𝑇2(𝑑𝑌2 + 𝑑𝑍2) (19) Case II:	cache/cana-5017.pdf	txt/cana-5017.txt