Hi Michael, I have a small comment. In page 2, the first phrase, you say that the k+ dN/dy distribution is wider than the pion distribution because strangeness is related to the net baryon density. We know that strange quarks are created in pairs both from the excited vacuum or from rescaterrings (quark-antiquark and hadronic channels). So, i think that there are 2 reasons for the wider K+ distribution: 1.) memory effect due to the contained up quark; and 2) rescatterings create extra strange quarks with a non-gaussian distribution. The memory effect affects also the pions so actually is not producing a bigger width for kaons. In my opinion, the extra kaonic width is due to the rescatterings which depend on the baryonic density, not on the net-baryonic density. I looked over lower energy data (e.g. top AGS, SPS) and i observed that the K+/pi+ ratio follows a dependence with the density of protons. Especially in the SPS Pb+Pb_at_158GeV data, one can observe how the K+/pi+ ratio follows the fragmentation peak. I'll show some figures in the next days since i am preparing the article and the abstract for QM08. Regards, Ionut > Dear Brahmin, > attached are my (very late) proceedings for SQM07. I > would be very interested in your timely comments. > Michael + 1 785 550 8835 > _______________________________________________ > Brahms-l mailing list > Brahms-l_at_lists.bnl.gov > https://lists.bnl.gov/mailman/listinfo/brahms-l > -- 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 Wed Oct 24 2007 - 10:15:10 EDT
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