From spinning to non-spinning cosmic string spacetimes
arXiv:gr-qc/9908003 · doi:10.1088/0264-9381/16/10/302
Abstract
We analyse the properties of a fluid generating a spinning cosmic string spacetime with flat limiting cases corresponding to a constant angular momentum in the infinite past and static configuration in the infinite future. The spontaneous loss of angular momentum of a spinning cosmic string due to particle emission is discussed. The rate of particle production between the spinning and non-spinning cosmic string spacetimes is calculated.
11 pages, 1 figure, LaTeX To appear in Class. Quantum Grav
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