On the possibility of the condensation of the charged rho-meson field in dense isospin asymmetric baryon matter

Details On the possibility of the condensation of the charged rho-meson field in dense isospin asymmetric baryon matter On the possibility of the condensation of the charged rho-meson field in dense isospin asymmetric baryon matter

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phlb..392..262v&link_type=abstract

Physics Letters B, v. 392, p. 262-266.

Physics

17

Scientific paper

It is shown that at sufficiently large density the isospin-asymmetric baryon matter may undergo the phase transition to the ρ-condensate state being characterized by the finite values of the charged ρ-meson mean fields. The appearance of such a condensate diminishes the asymmetry energy of the baryon matter. It is shown that in the neutron stars the corresponding phase transition is of the first order. Possible consequences are enumerated.

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