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Magnetic field of pulsars with superconducting quark core

Published online by Cambridge University Press:  12 April 2016

David Blaschke
Affiliation:
Fachbereich Physik, Universität Rostock, Universitätsplatz 1, D–18051 Rostock, Germany
David M. Sedrakian
Affiliation:
Physics Department, Yerevan State University, Alex Manoogian Str. 1, 375025 Yerevan, Armenia
Karen M. Shahabasyan
Affiliation:
Physics Department, Yerevan State University, Alex Manoogian Str. 1, 375025 Yerevan, Armenia

Abstract

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Within recent nonperturbative approaches to the effective quark interaction the diquark condensate forms a superconductor of second kind. Therefore the magnetic field will not be expelled from the superconducting quark core in accordance with observational data which indicate that life times of pulsar magnetic fields exceed 107 years.

Type
Part 9. Population and Neutron Star Properties
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Berges, J. & Rajagopal, K. 1999, Nucl. Phys. B, 538, 215 CrossRefGoogle Scholar
Bailin, D. & Love, A. 1984, Phys. Rep., 107, 325 CrossRefGoogle Scholar
Blaschke, D., Sedrakian, D.M. & Shahabasyan, K.M. 1999, astro-ph/9904395Google Scholar
Glendenning, N.K., 1992, Phys. Rev. D, 46, 1274 CrossRefGoogle Scholar
Makashima, K. 1992, in: The structure and evolution of neutron stars, eds. Pines, D., Tamagaki, R. & Tsuruta, S. (Addison-Wesley), 86 Google Scholar
Sedrakian, D.M. & Shahabasian, K.M. 1980, Astrofizika, 16, 417 Google Scholar
Sedrakian, A.D. & Sedrakian, D.M. 1995, ApJ, 447, 305 CrossRefGoogle Scholar
Wilczek, F. 1999, hep-ph/9908480Google Scholar