Physics – Nuclear Physics – Nuclear Theory
Scientific paper
2002-09-24
Phys.Rev.C67:014904,2003
Physics
Nuclear Physics
Nuclear Theory
46 pages, including 15 eps figures, to be published in Phys. Rev. C
Scientific paper
10.1103/PhysRevC.67.014904
We calculate $p, \pi^\pm, K^\pm$ and $\Lambda$(+$\Sigma^0$) rapidity distributions and compare to experimental data from SIS to SPS energies within the UrQMD and HSD transport approaches that are both based on string, quark, diquark ($q, \bar{q}, qq, \bar{q}\bar{q}$) and hadronic degrees of freedom. The two transport models do not include any explicit phase transition to a quark-gluon plasma (QGP). It is found that both approaches agree rather well with each other and with the experimental rapidity distributions for protons, $\Lambda$'s, $\pi^\pm$ and $K^\pm$. Inspite of this apparent agreement both transport models fail to reproduce the maximum in the excitation function for the ratio $K^+/\pi^+$ found experimentally between 11 and 40 A$\cdot$GeV. A comparison to the various experimental data shows that this 'failure' is dominantly due to an insufficient description of pion rapidity distributions rather than missing 'strangeness'. The modest differences in the transport model results -- on the other hand -- can be attributed to different implementations of string formation and fragmentation, that are not sufficiently controlled by experimental data for the 'elementary' reactions in vacuum.
Bratkovskaya Elena L.
Cassing Wolfgang
Stoecker Horst
Weber Harald
No associations
LandOfFree
Hadronic observables from SIS to SPS energies - anything strange with strangeness ? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Hadronic observables from SIS to SPS energies - anything strange with strangeness ?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hadronic observables from SIS to SPS energies - anything strange with strangeness ? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-612831