Abstract
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.
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© 1995 Springer-Verlag
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de Freitas Pacheco, J.A. (1995). Dibaryons in dense nuclear matter. In: Roxburgh, I.W., Masnou, JL. (eds) Physical processes in astrophysics. Lecture Notes in Physics, vol 458. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0118722
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DOI: https://doi.org/10.1007/BFb0118722
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