Non-axisymmetric oscillations of differentially rotating relativistic stars
Passamonti, Andrea, Stavridis, Adamantios and Kokkotas, Kostas D. (2008) Non-axisymmetric oscillations of differentially rotating relativistic stars. Physical Review D, 77, (2), 024029-[14pp]. (doi:10.1103/PhysRevD.77.024029).
Full text not available from this repository.
Non-axisymmetric oscillations of differentially rotating stars are studied using both slow rotation and Cowling approximation. The equilibrium stellar models are relativistic polytropes where differential rotation is described by the relativistic j-constant rotation law. The oscillation spectrum is studied versus three main parameters: the stellar compactness M/R, the degree of differential rotation A and the number of maximun couplings [script-I]max. It is shown that the rotational splitting of the non-axisymmetric modes is strongly enhached by increasing the compactness of the star and the degree of differential rotation. Finally, we investigate the relation between the fundamental quadrupole mode and the corotation band of differentially rotating stars.
|Keywords:||spectral properties of differentially rotating neutron stars.|
|Subjects:||Q Science > QB Astronomy
Q Science > QC Physics
|Divisions:||University Structure - Pre August 2011 > School of Mathematics > Applied Mathematics
|Date Deposited:||17 Sep 2008|
|Last Modified:||02 Mar 2012 13:11|
|Contributors:||Passamonti, Andrea (Author)
Stavridis, Adamantios (Author)
Kokkotas, Kostas D. (Author)
|Date:||17 January 2008|
|Contact Email Address:||A.Passamonti@soton.ac.uk|
|RDF:||RDF+N-Triples, RDF+N3, RDF+XML, Browse.|
Actions (login required)