Thermal evolution of neutron stars described within the equation of state with induced surface tension
- 31 January 2021
- journal article
- research article
- Published by Wiley in Astronomische Nachrichten
- Vol. 342 (1-2), 332-336
- https://doi.org/10.1002/asna.202113929
Abstract
No abstract availableKeywords
This publication has 30 references indexed in Scilit:
- Relativistic Shapiro delay measurements of an extremely massive millisecond pulsarNature Astronomy, 2019
- Cooling of the Cassiopeia A neutron star and the effect of diffusive nuclear burningPublished by AIP Publishing ,2019
- Influence of flow constraints on the properties of the critical endpoint of symmetric nuclear matterPhysical Review C, 2018
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star InspiralPhysical Review Letters, 2017
- Statistical theory of thermal evolution of neutron starsMonthly Notices of the Royal Astronomical Society, 2014
- A Massive Pulsar in a Compact Relativistic BinaryScience, 2013
- A neutron star with a carbon atmosphere in the Cassiopeia A supernova remnantNature, 2009
- Pairing gaps in nucleonic superfluidsNuclear Physics A, 1993
- Superfluidity of neutron matterNuclear Physics A, 1985
- Theory of SuperconductivityPhysical Review B, 1957