Perfect Fluid Cosmological Model In Presence Of Electromagnetic Field
Properties of a non-static cylindrically symmetric cosmological model with an electromagnetic field
Keywords:
perfect fluid, cosmological model, electromagnetic field, homogeneous, non-degenerate, Petrov type-I, energy momentum tensor, physical properties, geometrical properties, pressure, density, scalar of expansion, shearAbstract
In this paper, we have constructed a non-static cylindrically symmetric cosmological modelwhich is specially homogeneous non-degenerate Petrov type-I. the energy momentum tensor has beenassumed to be that of a perfect fluid with an electromagnetic field and the 4-current is either zero orspace-tike. Various physical and geometrical properties like pressure, density, scalar of expansion andshear etc have been found and discussedPublished
2022-12-01
How to Cite
[1]
“Perfect Fluid Cosmological Model In Presence Of Electromagnetic Field: Properties of a non-static cylindrically symmetric cosmological model with an electromagnetic field”, JASRAE, vol. 19, no. 6, pp. 335–339, Dec. 2022, Accessed: Jul. 01, 2024. [Online]. Available: https://ignited.in/jasrae/article/view/14188
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How to Cite
[1]
“Perfect Fluid Cosmological Model In Presence Of Electromagnetic Field: Properties of a non-static cylindrically symmetric cosmological model with an electromagnetic field”, JASRAE, vol. 19, no. 6, pp. 335–339, Dec. 2022, Accessed: Jul. 01, 2024. [Online]. Available: https://ignited.in/jasrae/article/view/14188