The r-mode instability in rotating neutron stars

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 particu...

Full description

Bibliographic Details
Main Authors: Andersson, Nils (Author), Kokkotas, Kostas D. (Author)
Format: Article
Language:English
Published: 2001.
Subjects:
Online Access:Get fulltext
Description
Summary: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.