Post-Minkowskian analysis of slowly rotating stars
The formalism developed by Hartle is used to set up the fieldequations of slowly and rigidly rotating stars valid to secondorder in the rotation parameter. These equations are then solvedin the exterior vacuum region. In the interior region the fieldequations cannot be solved analytically and an exp...
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| Format: | Others |
| Language: | English |
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Umeå universitet, Institutionen för fysik
2010
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| Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-37486 |