Strange hadron matter and SU ( 3 ) symmetry

We calculate saturation curves for strange hadron matter using recently constructed baryon-baryon potentials which are constrained by SU(3) symmetry. All possible interaction channels within the baryon octet (consisting of N , Λ, Σ, and Ξ) are considered. It is found that a small Λ fraction in nuclear matter slightly increases binding, but that larger fractions (> 10%) rapidly cause a decrease. Charge-neutral {N,Λ,Ξ} systems, with equal densities for nucleons and cascades, are only very weakly bound. The dependence of the binding energies on the strangeness per baryon, fs, is predicted for various {N,Λ,Ξ} and {N,Λ,Σ,Ξ} systems. The implications of our results in relativistic heavy-ion collisions and the core of a dense star are discussed. We also discuss the differences between our results and previous hadron matter calculations. 21.65.+f, 13.75.Ev, 12.39.Pn, 21.30.-x Typeset using REVTEX