Superfluid instability of r-modes in "differentially rotating" neutron stars (2013)
Attributed to:
Modelling compact objects for precision astrophysics
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1103/physrevd.87.063007
Publication URI: http://dx.doi.org/10.1103/physrevd.87.063007
Type: Journal Article/Review
Parent Publication: Physical Review D
Issue: 6
ISSN: 1550-7998