
Bianchi-VI inflationary model with flat potential in general relativity
Author(s) -
Sathyashankara Sharma,
Laxmi Poonia,
Sunil Kumawat
Publication year - 2021
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1921/1/012130
Subject(s) - algorithm , physics , computer science
We have investigated Bianchi Type VI inflationary model in presence of flat potential to study the accelerating behavior of the physical universe in detail. To obtain the deterministic solution we consider the supplementary relation the component σ 3 3 of shear tensor σ j i is proportional to expansion parameter θ which yield to appropriate condition c = ( ab ) N between metric coefficients, where N is non-negative constant. Special case in Bianchi Type VI model provide Bianchi I, III and V space-time. Geometrical and dynamical aspects of models are also discussed in different cases