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...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
2001.
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| Subjects: | |
| Online Access: | Get fulltext |
| LEADER | 00860 am a22001333u 4500 | ||
|---|---|---|---|
| 001 | 29439 | ||
| 042 | |a dc | ||
| 100 | 1 | 0 | |a Andersson, Nils |e author |
| 700 | 1 | 0 | |a Kokkotas, Kostas D. |e author |
| 245 | 0 | 0 | |a The r-mode instability in rotating neutron stars |
| 260 | |c 2001. | ||
| 856 | |z Get fulltext |u https://eprints.soton.ac.uk/29439/1/29439.pdf | ||
| 520 | |a 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. | ||
| 655 | 7 | |a Article | |