Non-radial oscillations of neutron stars and the detection of gravitational waves
classification
🌀 gr-qc
keywords
gravitationalstarsf-modesneutronnon-radialoscillationswavebelieved
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We study the non-radial oscillations of relativistic neutron stars, in particular the (fundamental) f-modes, which are believed to be the most relevant for the gravitational wave emission of perturbed isolated stars. The expected frequencies of the f-modes are compared to the sensitivity range of Mario Schenberg, the Brazilian gravitational wave spherical detector.
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