Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/10879
Citations | ||
Scopus | Web of Science® | Altmetric |
---|---|---|
?
|
?
|
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Stoks, V. G. J. | en |
dc.contributor.author | Lee, T-S. H. | en |
dc.date.issued | 1999 | en |
dc.identifier.citation | Physical Review C, 1999; 60(2):024006 | en |
dc.identifier.issn | 0556-2813 | en |
dc.identifier.uri | http://hdl.handle.net/2440/10879 | - |
dc.description.abstract | 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. | en |
dc.description.statementofresponsibility | V. G. J. Stoks, and T.-S. H. Lee | en |
dc.language.iso | en | en |
dc.publisher | American Physical Society | en |
dc.rights | © 1999 The American Physical Society | en |
dc.title | Strange hadron matter and SU(3) symmetry | en |
dc.type | Journal article | en |
dc.contributor.school | School of Chemistry and Physics | en |
dc.identifier.doi | 10.1103/PhysRevC.60.024006 | en |
Appears in Collections: | Special Research Centre for the Subatomic Structure of Matter publications |
Files in This Item:
File | Size | Format | |
---|---|---|---|
hdl_10879.pdf | 144.88 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.