Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 442, Issue 1, Pages L90-L94Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnrasl/slu061
Keywords
stars: interiors; stars: neutron; stars: oscillations (including pulsations)
Categories
Funding
- RFBR [14-02-00868-a, 14-02-31616-mol-a]
- RF president programme [MK-506.2014.2, NSh-294.2014.2]
Ask authors/readers for more resources
We demonstrate a possibility of existence of peculiar temperature-dependent composition g modes in superfluid neutron stars. We calculate the Brunt-Vaisala frequency for these modes, as well as their eigenfrequencies. The latter turn out to be rather large, up to similar to 500 Hz for a chosen model of a neutron star. This result indicates, in particular, that use of the barotropic equation of state may be not a good approximation for calculation of inertial modes even in most rapidly rotating superfluid neutron stars.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available