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Paper detail

From spinning to non-spinning cosmic string spacetimes

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.

preprint1999arXivOpen access
V. A. De LorenciR. D. M. De PaolaN. F. Svaiter
gr-qc
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V. A. De LorenciR. D. M. De PaolaN. F. Svaiter

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