785 864 3949, cell 785 550 8835 -----Original Message----- From: Murray, Michael J Sent: Sat 6/23/2007 3:54 PM To: brahms-l_at_lists.bnl.gov Subject: Michael's preliminary SQM07 talk Dear Friends, I have uploaded a draft of my SQM 2007 talk to the collaboration meeting agenda page http://indico.cern.ch/conferenceDisplay.py?confId=17731 (It was too large to send out via brahms-l). The files is at the top of the page under "MATERIAL" I am trying to coordinate with Pawel though there is some overlap. The main point I am trying to make is that our particle yields can be descrbed by both limiting fragmenation and thermal descriptions with baryon density or baryon chemical potential being a very important parameter. Our flow measurements suggest that the system thermalizes very early at all rapidities. We need a way to thermalize the system very early but the state of the system depends on the baryons in it. One such mechanism is the "charged white hole" hypothesis of Satz, Karhzeev et al. The change in temperature from Y=3 at 200GeV to y=0 at 62 GeV is consistent with this idea but I don't think the rather slow drop of T with rapidity at /s=62GeV is. Anyway here is my talk and I would be very glad to receive any comments. Thanks for making BRAHMS a great experiment. Michael _______________________________________________ Brahms-l mailing list Brahms-l_at_lists.bnl.gov https://lists.bnl.gov/mailman/listinfo/brahms-lReceived on Sat Jun 23 2007 - 17:04:03 EDT
This archive was generated by hypermail 2.2.0 : Sat Jun 23 2007 - 17:04:31 EDT