Journal of Siberian Federal University. Mathematics & Physics / Two Fluid Scenario Dark Energy Cosmological Model with Linearly Varying Deceleration Parameter in Lyra’s Geometry

Full text (.pdf)
Issue
Journal of Siberian Federal University. Mathematics & Physics. Prepublication
Authors
Mandala Krishna; SobhanBabu Koppala; Santhikumar Rajamahanthi
Contact information
Mandala Krishna: Raghu Engineering College Visakhapatnam, AndhraPradesh, India-531162; mandala.krishna.phd@gmail.com OCRID: 0000-0003-1975-8930; SobhanBabu Koppala: University Collage of Engineering Kakinada Narasaraopeta, AndhraPradesh, India-522616; ksobhanjntu@gmail.com OCRID: 0000-0002-2991-7651; Rajamahanthi Santhikumar: Aditya Institute of Technology and Management K.Kotturu, Tekkali, Srikakulam Dist, Andhrapradesh-532201, India; skrmahanthi@gmail.com OCRID: 0000-0001-5122-3800
Keywords
dark energy; two fluid scenario; barotropic; Lyra’s geometry
Abstract

In this paper, we explore the evaluation of the dark energy parameter within a spatially homogeneous and anisotropic Bianchi type-V I0 spacetime, incorporating Lyra geometry. To obtain a determinate solution, we solve the field equations using the linearly varying deceleration parameter pro- posed by Akarsu and Dereli (2012). We analyze two scenarios involving interacting and non-interacting fluids (barotropic and dark energy) and derive general results for each case. The physical implications of these findings are also discussed

Pages
519–531
EDN
QRNGKM
Paper at repository of SibFU
https://elib.sfu-kras.ru/handle/2311/156164
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