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The quadrupole moment of slowly rotating stars
Umeå University, Faculty of Science and Technology, Department of Physics.
KFKI Research Institute for Particle and Nuclear Physics, Budapest.
2010 (English)In: / [ed] Ruth Lazkoz and Raül Vera, IOPScience , 2010, Vol. 229, no 1, 012025- p.Conference paper, Published paper (Refereed)
Abstract [en]

The second order field equations for the interior of slowly and rigidly rotating stars are solved numerically for different classes of possible equations of state and these solutions are then matched to the general asymptotically flat axisymmetric vacuum metric to second order in the rotational parameter. For these solutions we find that the quadrupole moment differs from that of the Kerr metric. Further we consider the post-Minkowskian limit analytically.

Place, publisher, year, edition, pages
IOPScience , 2010. Vol. 229, no 1, 012025- p.
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:umu:diva-34849DOI: 10.1088/1742-6596/229/1/012025ISI: 000287182000025OAI: oai:DiVA.org:umu-34849DiVA: diva2:325981
Conference
Spanish Relativity Meeting ERE 2009
Note

Conference: Spanish Relativity Meeting ERE from the 7th to 11th September 2009, Bilbao

Available from: 2010-06-21 Created: 2010-06-21 Last updated: 2016-05-25Bibliographically approved

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