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Critical gravitational collapse with angular momentum

Aug 1, 2016

9 pages

Published in:

Phys.Rev.D 94 (2016) 8, 084012

Published: Oct 6, 2016

e-Print:

1608.00491 [gr-qc]

DOI:

10.1103/PhysRevD.94.084012

View in:

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Abstract: (APS)

We derive a theoretical model of mass and angular momentum scaling in type-II critical collapse with rotation. We focus on the case where the critical solution has precisely one, spherically symmetric, unstable mode. We demonstrate agreement with numerical results for critical collapse of a rotating radiation fluid, which falls into this case.

Note:

Version accepted for publication in PRD

References(21)

Figures(9)

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