Tkachenko modes in rotating neutron stars: The effect of compressibility and implications for pulsar timing noise (2011)

First Author: Haskell B

Attributed to: Sources for gravitational wave astronomy funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1103/physrevd.83.043006

Publication URI: http://dx.doi.org/10.1103/physrevd.83.043006

Type: Journal Article/Review

Parent Publication: Physical Review D

Issue: 4

ISSN: 1550-7998