• REENA MEHTA
• Preeti Mehta

Bianchi type-VI0 magnetized cosmological models with a time-dependent displacement field for stiff fluid distribution within the framework of Lyra geometry are investigated. To get the deterministic model of the universe, we have assumed that shear tensor () is proportional to the expansion scalar () which leads to A = Bn, where A and B are metric functions and n is a positive constant. The physical and geometrical aspects of the models are also discussed.

Bianchi type-VI0, Cosmological models, Magnetized, Stiff fluid, Lyra's geometry.

"BIANCHI TYPE-VI0 MAGNETIZED STIFF FLUID COSMOLOGICAL MODELS IN LYRA'S GEOMETRY", International Journal of Emerging Technologies and Innovative Research (www.jetir.org), ISSN:2349-5162, Vol.6, Issue 6, page no.852-861, August-2019, Available :http://www.jetir.org/papers/JETIR1907118.pdf

"BIANCHI TYPE-VI0 MAGNETIZED STIFF FLUID COSMOLOGICAL MODELS IN LYRA'S GEOMETRY", International Journal of Emerging Technologies and Innovative Research (www.jetir.org | UGC and issn Approved), ISSN:2349-5162, Vol.6, Issue 6, page no. pp852-861, August-2019, Available at : http://www.jetir.org/papers/JETIR1907118.pdf