Axially magnetized dark energy cosmological model
2019 ◽
Vol 34
(27)
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pp. 1950217
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Keyword(s):
Big Rip
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We investigate the behavior of the skewness parameters for an anisotropic universe in the framework of General Relativity. Non-interacting dark energy is considered in presence of electromagnetic field. A time-varying deceleration parameter simulated by a hybrid scale factor is considered. The dynamics of the universe is investigated in presence and absence of magnetic field. The equation of state parameter of dark energy evolves within the range predicted by the observations. Magnetic field is observed to have a substantial effect on the cosmic dynamics and the skewness parameters. The models discussed here end in a big rip and become isotropic at finite time.
2019 ◽
Vol 34
(30)
◽
pp. 1950184
2015 ◽
Vol 24
(07)
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pp. 1550048
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2005 ◽
Vol 14
(02)
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pp. 355-362
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2013 ◽
Vol 91
(4)
◽
pp. 351-354
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Keyword(s):
2021 ◽
Vol 42
(1)
◽
pp. 39-57
2019 ◽
Vol 79
(11)
◽
Keyword(s):