Stellar Pulsations excited by a scattered mass

Details Stellar Pulsations excited by a scattered mass Stellar Pulsations excited by a scattered mass

1999-01-22

arxiv.org/abs/gr-qc/9901060v1

Phys.Rev. D59 (1999) 124020

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

23 pages, 6 figures, RevTeX

Scientific paper

10.1103/PhysRevD.59.124020

We compute the energy spectra of the gravitational signals emitted when a
mass m is scattered by the gravitational field of a star of mass M >> m. We
show that, unlike black holes in similar processes, the quasi-normal modes of
the star are excited, and that the amount of energy emitted in these modes
depends on how close the exciting mass can get to the star.

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