Comment on “Gravitational Radiation Instability in Hot Young Neutron Stars”
- 12 February 2001
- journal article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 86 (7) , 1384
- https://doi.org/10.1103/physrevlett.86.1384
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- A numerical study of the r-mode instability of rapidly rotating nascent neutron starsMonthly Notices of the Royal Astronomical Society, 2000
- [CLC][ITAL]r[/ITAL][/CLC]-Mode Runaway and Rapidly Rotating Neutron StarsThe Astrophysical Journal, 2000
- First order kaon condensatePhysical Review C, 1999
- Gravitational Radiation Limit on the Spin of Young Neutron StarsThe Astrophysical Journal, 1999
- Onset of hyperon formation in neutron star matter from Brueckner theoryPhysical Review C, 1998
- How to Identify a Strange StarPhysical Review Letters, 1998
- Gravitational waves from hot young rapidly rotating neutron starsPhysical Review D, 1998
- Gravitational Radiation Instability in Hot Young Neutron StarsPhysical Review Letters, 1998
- Astrophysical significance of the dissipation of turbulence in a dense baryon fluidProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1971
- Effects of hyperons on the vibrations of neutron starsAstrophysics and Space Science, 1969