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The r-mode instability in rotating neutron stars

N. Andersson·K. D. Kokkotas
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Abstract

In this review we summarize the current understanding of the gravitational-wave driven instability associated with the so-called r-modes in rotating neutron stars. We discuss the nature of the r-modes, the detailed mechanics of the instability and its potential astrophysical significance. In particular we discuss results regarding the spin-evolution of nascent neutron stars, the detectability of r-mode gravitational waves and mechanisms limiting the spin-rate of accreting neutron stars in binary systems.

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BibTeXRIS

N. Andersson, K. D. Kokkotas. 2000-10-27. The r-mode instability in rotating neutron stars. https://doi.org/10.1142/s0218271801001062

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