Variation in Magnetic Field Strength During a Specific Anisotropic Gravitational Collapse
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The MHD approximation has been made in general relativity to derive expressions in terms of the fluid's total proper energy density and rest-mass density for the variation in the strength of the magnetic field during the anisotropic gravitational collapse in which the condition ?ab HaHb = 0 holds throughout the collapse, where ?ab is the expansion tensor. The physical significance of this condition is also examined.
1976 ◽
Vol 32
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pp. 613-622
2021 ◽
pp. 1045389X2110643
2003 ◽
Vol 13
(12)
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pp. 3783-3789
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2019 ◽
Vol 21
(25)
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pp. 13696-13705
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2013 ◽
Vol 7
(2)
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pp. 216-220
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