LRS Bianchi type II stiff fluid inflationary model with flat potential in general relativity

In the current research, I have used the framework of Bianchi Type II LRS type metric using the condition of the stiff fluid inflationary model with flat potential. For a relativistic solution of the field equation, we have assumed an auxiliary condition R = Sm between the metric potential R & S., where m is a constant, which can take any value apart from one. For a stiff fluid, apply the equation of state p=ρ . Some dynamic feature of the model is also discussed. The physical parameters are also illustrated through graphical representations.

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Publication Details

Journal
Journal of Interdisciplinary Mathematics
Published
2025-01-01
DOI
https://doi.org/10.47974/jim-2375
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.00
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article

LRS Bianchi type II stiff fluid inflationary model with flat potential in general relativity

Manali Vijayvargiya, Varsha Maheshwari, Laxmi Poonia, Rakhi Mathur
Journal of Interdisciplinary Mathematics
Cosmology and Gravitation Theories
article

LRS Bianchi type II stiff fluid inflationary model with flat potential in general relativity

Manali Vijayvargiya, Varsha Maheshwari, Laxmi Poonia, Rakhi Mathur
article en

Abstract

In the current research, I have used the framework of Bianchi Type II LRS type metric using the condition of the stiff fluid inflationary model with flat potential. For a relativistic solution of the field equation, we have assumed an auxiliary condition R = Sm between the metric potential R & S., where m is a constant, which can take any value apart from one. For a stiff fluid, apply the equation of state p=ρ . Some dynamic feature of the model is also discussed. The physical parameters are also illustrated through graphical representations.

Journal of Interdisciplinary MathematicsVol. 28(6)
Openalex Percentile: Top 81%
Cosmology and Gravitation Theories
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