2000
DOI: 10.1103/physrevd.62.124001
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Gravitational collapse of cylindrical shells made of counterrotating dust particles

Abstract: The general formulas of a non-rotating dynamic thin shell that connects two arbitrary cylindrical regions are given using Israel's method. As an application of them, the dynamics of a thin shell made of counter-rotating dust particles, which emits both gravitational waves and massless particles when it is expanding or collapsing, is studied. It is found that when the models represent a collapsing shell, in some cases the angular momentum of the dust particles is strong enough to halt the collapse, so that a sp… Show more

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Cited by 36 publications
(3 citation statements)
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References 24 publications
(31 reference statements)
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“…In more realistic situations, the spacetime has neither cylindrical symmetry nor zero angular momentum, and gravitational and particle radiations are always expected to occur. In particular, when radiation is taken into account, modeled by an outgoing radiation fluid [216], Pereira and Wang found [261] that similar results to a rotating spheroid obtained in [283] also hold for a collapsing cylindrical shell made of counterrotating dust particles: in some cases the angular momentum of the dust particles is strong enough to halt the collapse, so that a spacetime singularity is prevented from forming, while in other cases it is not, and a line-like spacetime singularity is finally formed on the symmetry axis.…”
Section: Gravitational Collapse and Emission Of Gravitational Wavesmentioning
confidence: 99%
“…In more realistic situations, the spacetime has neither cylindrical symmetry nor zero angular momentum, and gravitational and particle radiations are always expected to occur. In particular, when radiation is taken into account, modeled by an outgoing radiation fluid [216], Pereira and Wang found [261] that similar results to a rotating spheroid obtained in [283] also hold for a collapsing cylindrical shell made of counterrotating dust particles: in some cases the angular momentum of the dust particles is strong enough to halt the collapse, so that a spacetime singularity is prevented from forming, while in other cases it is not, and a line-like spacetime singularity is finally formed on the symmetry axis.…”
Section: Gravitational Collapse and Emission Of Gravitational Wavesmentioning
confidence: 99%
“…Nakao and Morisawa [14,15] introduced a an isotropic scheme and investigated cylindrical collapse for dust and perfect fluid, respectively. Cylindrical symmetric gravitational collapse of counter rotating dust shells can be found in the [16,17], axially symmetric vacuum solution [18], and cylindrical symmetric collapse in anisotropic in [7]. An axially symmetric null dust gravitational collapse has been discussed in [19].…”
Section: Introductionmentioning
confidence: 95%
“…Nakao and Morisawa [36] studied the high-speed collapse of cylindrically symmetric thick shell composed of dust and perfect fluid with nonvanishing pressure [37]. Recent work describes the cylindrically symmetric collapse of counterrotating dust shells [38][39][40], self-similar scalar field [41], axially symmetric vacuum space-time [42], and a cylindrically symmetric anisotropic fluid space-time [43]. Some other examples of nonspherical gravitational collapse would be discussed in [44][45][46][47][48][49][50][51][52][53].…”
Section: Introductionmentioning
confidence: 99%