E N Glass and J P Krisch 2004 Class. Quantum Grav. 21 5543 doi:10.1088/0264-9381/21/23/015
Spinning up asymptotically flat spacetimes
E N Glass and J P Krisch
Show affiliationsWe present a method for constructing stationary, asymptotically flat, rotating solutions of Einstein's field equations. One of the spun-up solutions has quasilocal mass but no global mass. It has an ergosphere but no event horizon. The angular momentum is constant everywhere beyond the ergosphere. The energy–momentum content of this solution can be interpreted as a rotating string fluid.
- PACS
- MSC
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83C05 Einstein's equations (general structure, canonical formalism, Cauchy problems)
- Subjects
- Dates
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Issue 23 (7 December 2004)
Received 26 January 2004, in final form 23 September 2004
Published 16 November 2004
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Spinning up asymptotically flat spacetimes
E N Glass and J P Krisch 2004 Class. Quantum Grav. 21 5543
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