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- Study of gravitational waves from stable/unstable neutron star models
- Further development of perturbative techniques to infer detailed information about GW sources i.e. mass, radius,
rotational rate and, in the case of NS, the EOS of the final object.
- Development of perturbation equations for slowly rotating stars for numerical time evolutions. Generic initial data will
then be evolved, with special focus on the various pulsation modes of the system.
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This work has been supported by the EU Programme
'Improving the Human Research Potential and the
Socio-Economic Knowledge Base' (Research Training Network
Contract HPRN-CT-2000-00137).
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