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Scattering of particles by neutron stars: Time-evolutions for axial perturbations

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arxiv gr-qc/0008057 v1 pith:YWP7BRMS submitted 2000-08-23 gr-qc astro-ph

Scattering of particles by neutron stars: Time-evolutions for axial perturbations

V.Ferrari (Rome) , K.D.Kokkotas (Thessaloniki) This is my paper
classification gr-qc astro-ph
keywords particlesaxialscatteringstarsadditionbinarycapturecomplicated
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The excitation of the axial quasi-normal modes of a relativistic star by scattered particles is studied by evolving the time dependent perturbation equations. This work is the first step towards the understanding of more complicated perturbative processes, like the capture or the scattering of particles by rotating stars. In addition, it may serve as a test for the results of the full nonlinear evolution of binary systems.

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Cited by 4 Pith papers

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