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The Neutron Stars with Magnetic Charges

Published online by Cambridge University Press:  04 August 2017

Y.-J. Wang  and
Q.-H. Peng
Y.-J. Wang
Affiliation:
Astrophys. Dept., Changsha Railway Inst., Changsha, China
Q.-H. Peng
Affiliation:
Astrophys. Inst., Nanjing Univ., Nanjing, China

Extract

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From KNK metric, we have shown that there may exist some kind of celestial bodies which can not collapse to black holes provided that the proportion of the content of the magnetic monopoles to the nuclei ξ = Nm/NB exceeds a critical value ξc (l-a2/Rg2), in which ξc =√G mB/gm ∼ 4.4 ×1021, a = J/Mc, Rg =GM/c2.

Type
V. Neutron Star Physics
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 460
Copyright
Copyright © Reidel 1987