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Lee-Wick Model and Soliton Stars

  • R. Vinh Mau
Part of the NATO ASI Series book series (NSSB, volume 223)

Abstract

Massive stars after exhausting their thermonuclear fuel die in supernovae explosions. Some residues of these massive stars become neutron stars with the following properties: mass ~ 1.4 m, radius ~ 10 km, large density.

Keywords

Black Hole Neutron Star Massive Star Supernova Explosion Fermion Number 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© Plenum Press, New York 1990

Authors and Affiliations

  • R. Vinh Mau
    • 1
    • 2
  1. 1.Division de Physique ThéoriqueI.P.N.Orsay CedexFrance
  2. 2.LPTPEUniversité P. et M. CurieParis Cedex 05France

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