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Nuclear Forces in High Density Matter

Published online by Cambridge University Press:  07 February 2017

M. R. McNaughton
M. R. McNaughton*
Affiliation:
Laboratory for Astrophysics and Space Research, Enrico Fermi Institute, Chicago, Ill., U.S.A.

Abstract

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The conditions for superfluidity or ferromagnetism in neutron stars are presented and discussed (but not derived). It is suggested that present estimates relating to these are in error and that the predictions made contradict at least one of three sets of nuclear physics data cited in the text. This is due to neglecting the action of the exclusion principle.

A comparatively simple method for calculating the strength of nuclear forces in the presence of many-body effects is outlined. Some preliminary results are presented together with projected future developments.

Type
Session 6
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 356 - 363
Copyright
Copyright © Reidel 1971 

References

Brownell, D. H. and Callaway, J. A.: 1969, Nuovo Cimento 60B, 169.CrossRefGoogle Scholar
Day, B. D.: 1967, Rev. Mod. Phys. 39, 719.Google Scholar
Hoffberg, M., Glassgold, A. E., Richardson, R. W., and Ruderman, M.: 1970, Phys. Rev. Letters 24, 775.CrossRefGoogle Scholar
McNaughton, M. R.: 1969, , .Google Scholar
Wang, C. G., Rose, W. K., and Schlenker, S. L.: 1970, Astrophys. J. 160, L17.CrossRefGoogle Scholar