期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 428, 期 1, 页码 L26-L30出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnrasl/sls007
关键词
stars: interiors; stars: neutron; stars: oscillations
资金
- Ministry of Education and Science of Russian Federation [11.G34.31.0001, 8409]
- RFBR [11-02-00253-a, 12-02-31270-mol-a]
- FASI [NSh-4035.2012.2]
- RF president programme [MK-857.2012.2]
- SPbSPU
We show that suppression of the baryon energy gaps, caused by the relative motion of superfluid and normal liquid components, can substantially influence dynamical properties and evolution of neutron stars. This effect has been previously ignored in the neutron star literature.
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