2017
DOI: 10.1155/2017/8786791
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A Study of Charged Cylindrical Gravitational Collapse with Dissipative Fluid

Abstract: The present works deals with gravitational collapse of cylindrical viscous heat conducting anisotropic fluid following the work of Misner and Sharp. Using Darmois matching conditions, the dynamical equations are derived and the effects of charge and dissipative quantities over the cylindrical collapse are analyzed. Finally, using the Miller-Israel-Steward causal thermodynamic theory, the transport equation for heat flux is derived and its influence on collapsing system has been studied.

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Cited by 5 publications
(2 citation statements)
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References 39 publications
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“…where E = Q(r) 2πR and Q(r) = 4π r 0 ζBRdr. The gravitational energy per specific length (also, known as C-energy) for cylindrical symmetric spacetime is given as follows [41,42]…”
Section: Viscous Dissipative Fluid Enclosed By Cylindrical Stellar Ob...mentioning
confidence: 99%
See 1 more Smart Citation
“…where E = Q(r) 2πR and Q(r) = 4π r 0 ζBRdr. The gravitational energy per specific length (also, known as C-energy) for cylindrical symmetric spacetime is given as follows [41,42]…”
Section: Viscous Dissipative Fluid Enclosed By Cylindrical Stellar Ob...mentioning
confidence: 99%
“…For cylindrically symmetric model with killing vectors, the circumference radius ρ and specific length l and areal radius r are defined as follows [41,42]…”
Section: Viscous Dissipative Fluid Enclosed By Cylindrical Stellar Ob...mentioning
confidence: 99%