Quasinormal Frequencies of (rotating) Black Holes (and Neutron Stars) as a Discrete Boundary Value Problem

Details Quasinormal Frequencies of (rotating) Black Holes (and Neutron Stars) as a Discrete Boundary Value Problem Quasinormal Frequencies of (rotating) Black Holes (and Neutron Stars) as a Discrete Boundary Value Problem

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.2353n&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

We propose to determine characteristic oscillation modes of rotating neutron stars by performing a mode analysis of linearized perturbations of the star, formulated as discretized boundary value problem. We describe results for a simple test problem, the quasinormal mode problem of a Schwarzschild black hole. We encounter surprising problems arising from additional modes of the discretized problem which tend to swamp the actual modes of the continuous system.

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