THE R-MODE INSTABILITY IN ROTATING NEUTRON STARS-Reference-Cited by-同舟云学术

THE R-MODE INSTABILITY IN ROTATING NEUTRON STARS

Published:2001-08 Issue:04 Volume:10 Page:381-441
ISSN:0218-2718
Container-title:International Journal of Modern Physics D
language:en
Short-container-title:Int. J. Mod. Phys. D

Author:

ANDERSSON NILS¹,KOKKOTAS KOSTAS D.²

Affiliation:

1. Department of Mathematics, University of Southampton, Southampton SO17 1BJ, UK

2. Department of Physics, Aristotle University of Thessaloniki, Thessaloniki 54006, Greece

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.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0218271801001062

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