Dear collaborator, Bellow find my draft for the QM08 abstract. I am grateful for comments and criticism. Regards, Ionut Title: "Strangeness production in Au+Au collisions at $\sqrt{s_{NN}}=62.4 GeV$" BRAHMS experiment has taken data from the short RHIC run for Au+Au collisions at c.m. energy of 62.4 AGeV. Due to its special setup, BRAHMS was able to measure and identify charged particles over the widest rapidity range at RHIC. This feature enabled us to shed some light on one of the predicted signals of quark gluon plasma (QGP), strangeness enhancement. Experimentally, we have a limited set of observables. BRAHMS can only measure charged pions, charged kaons, protons and anti-protons so the strange quarks that we can see are contained in the charged kaons. The majority of the produced strange quarks form negative kaons and $\Lambda$ baryons in comparable quantities so $K^{-}$ is not a good tool for strangeness estimation when we don't control the $\Lambda$ yield. The anti-strange quarks however form mostly positive kaons and $K^0$s in equal quantities. The other species containing anti-strange quarks are in a very limited number and this makes the number of positive kaons approximately proportional to the total strangeness created during the collision. From the AGS energies up to the highest RHIC energy we observed experimentally that the $K^{+}/\pi^{+}$ ratio is higher than the same ratio in p+p collisions at the same collision energy. This fact was interpreted to happen due to the final state effects (rescatterings) taking place in a nucleus-nucleus collision. We also observed that the difference between the strangeness ratio in nucleus-nucleus collisions and the one in p+p collisions is varying. By looking at older SPS data in mid-rapidity, together with BRAHMS data in different rapidity slices, we observed that there is a scaling of the $K^{+}/\pi^{+}$ ratio with the $\bar{p}/p$ ratio. Our conclusion is that in nucleus-nucleus collisions where the formed medium is baryon rich (e.g. AGS energies, low SPS energies, forward rapidity in Au+Au collisions at 62.4GeV in RHIC), the additional strangeness created trough rescatterings is higher than in the collisions where the medium created is highly deconfined and baryon poor (e.g. RHIC at 200GeV). A posible explanation might be the evolution time which is longer in low energy collisions and allows for multiple rescatterings before the chemical freezeout. In this work we will show measured yields and ratios of identified particles from the 10\% most central Au+Au collisions at 62.4 GeV together with comparisons with results from other experiments and from theoretical models. -- Ionut Cristian Arsene PhD student at Physics Department, University of Oslo, Norway Phone: +47 22856456 (Office) Phone: +47 94214593 (Mobile) _______________________________________________ Brahms-l mailing list Brahms-l_at_lists.bnl.gov https://lists.bnl.gov/mailman/listinfo/brahms-lReceived on Sun Oct 28 2007 - 11:47:13 EDT
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