Dibaryons in dense nuclear matter

  • J. A. de Freitas Pacheco
Contributed Papers
Part of the Lecture Notes in Physics book series (LNP, volume 458)


If interactions among H-particles can be described by a “hard-sphere” boson system, we find that a phase transition from nuclear to dibaryon matter may occur in massive neutron stars. The results depend also on the strong force coupling constant.


Neutron Star Nuclear Matter Baryon Density Strong Coupling Constant Density Jump 
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Copyright information

© Springer-Verlag 1995

Authors and Affiliations

  • J. A. de Freitas Pacheco
    • 1
  1. 1.Depto de AstronomiaUniversidade de São Paulo, IAGSão PauloBrazil

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