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Equation of state and pulsar death line
Published online by Cambridge University Press: 04 June 2018
Abstract
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In this proceeding, we are going to introduce our recent work about the dependence of pulsar death line on the equation of state (Zhou et al. 2017). The results show that the equation of state affects the location of the pulsar death line in the P-Ṗ diagram. We offer another point of view to understand the pulsar death line and multiple observational facts would help us to reveal the nature of pulsars.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 13 , Symposium S337: Pulsar Astrophysics the Next Fifty Years , September 2017 , pp. 432 - 433
- Copyright
- Copyright © International Astronomical Union 2018
References
Kaspi, V. M. & Kramer, M., 2016, preprint (arXiv: 1602.07738), Rapporteur talks in the Proceedings of the 26th Solvay Conference on Physics on Astrophysics and Cosmology, pp 22-61, World ScientificGoogle Scholar
Shapiro, S. L. & Teukolsky, S. A. 1983, Black Holes, White Dwarfs and Neutron Stars. The Physics of Compact Objects, Wiley Interscience, New YorkCrossRefGoogle Scholar