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Pulsar Glitches: Superfluid Unpinning

Published online by Cambridge University Press:  14 August 2015

P. W. Anderson ,
M. A. Alpar ,
D. Pines  and
J. Shaham
P. W. Anderson
Affiliation:
Bell Laboratories and Princeton University, New Jersey, USA
M. A. Alpar
Affiliation:
Bogazici University, Istanbul, Turkey
D. Pines
Affiliation:
University of Illinois, Urbana-Champaign, Illinois, USA
J. Shaham
Affiliation:
Racah Institute of Physics, Jerusalem, Israel

Extract

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In the neutron star crust, the neutron superfluid coexists with a lattice of nuclei. There are two different local densities of superfluid neutrons, inside and outside the nuclei, with a corresponding difference in the values of the superfluid gap and condensation energy.

Type
VI. Pulse Timing
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 299 - 300
Copyright
Copyright © Reidel 1981 

References

Hoffberg, M., Glassgold, A.E., Richardson, R.W., and Ruderman, M.: 1970, Phys. Rev. Letters 24, p. 775.Google Scholar
Negele, J.W. and Vautherin, D.: 1975, Nucl. Phys. A207, p. 298.Google Scholar
Takatsuka, T.: 1972, Prog. Theor. Phys. 48, p. 517.Google Scholar