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arXiv · gr-qc/9610035

Gravitational waves and pulsating stars: What can we learn from future observations?

Nils Andersson·Kostas D. Kokkotas
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Abstract

We present new results for pulsating stars in general relativity. First we show that the so-called gravitational-wave modes of a neutron star can be excited when a gravitational wave impinges on the star. Numerical simulations suggest that the modes may be astrophysically relevant, and we discuss whether they will be observable with future gravitational-wave detectors. We also discuss how such observations could lead to estimates of both the radius and the mass of a neutron star, and thus put constraints on the nuclear equation of state.

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Nils Andersson, Kostas D. Kokkotas. 1996-10-16. Gravitational waves and pulsating stars: What can we learn from future observations?. https://doi.org/10.1103/physrevlett.77.4134

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