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Distributional curvature of time dependent cosmic strings

Record type: Article

Colombeau's theory of generalized functions is used to calculate the contributions, at the rotation axis, to the distributional curvature for a time-dependent radiating cosmic string, and hence the mass per unit length of the string source. This mass per unit length is compared with the mass at null infinity, giving evidence for a global energy conservation law.

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Citation

Wilson, J.P. (1997) Distributional curvature of time dependent cosmic strings Classical and Quantum Gravity, 14, (12), pp. 3337-3351. (doi:10.1088/0264-9381/14/12/017).

More information

Published date: 1997
Additional Information: Received 16 May 1997, in final form 20 October 1997.

Identifiers

Local EPrints ID: 29344
URI: http://eprints.soton.ac.uk/id/eprint/29344
ISSN: 0264-9381
PURE UUID: b3b8bcf8-bf0b-4948-8d38-fc05d25779bc

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Date deposited: 27 Feb 2007
Last modified: 17 Jul 2017 15:58

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Author: J.P. Wilson

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