FYI -------------------------------------------- Flemming Videbaek Physics Department Bldg 510-D Brookhaven National Laboratory Upton, NY11973 phone: 631-344-4106 cell: 631-681-1596 fax: 631-344-1334 e-mail: videbaek @ bnl.gov ----- Original Message ----- From: "Timothy Hallman" <hallman@bnl.gov> To: "'Bond, Peter D'" <bond@bnl.gov>; "William A Zajc" <zajc@bnl.gov>; "Videbaek, Flemming" <videbaek@bnl.gov>; "'Wit Busza'" <busza@MIT.EDU> Cc: "Hallman" <hallman@bnl.gov> Sent: Wednesday, May 10, 2006 2:49 PM Subject: New STAR Paper on Scaling Properties of Hyperon Production in AuAu at 200 GeV > > Dear Peter, Bill, Flemming, and Wit: > > It is my pleasure to announce STAR's intention to submit the > following paper to Physical Review Letters in one week's time: > > "Scaling Properties of Hyperon Production in Au+Au > Collisions at \sqrt{s_{NN}} = 200 GeV". > > The abstract is enclosed. > > Sincerely, > > Tim Hallman > > > We present the scaling properties of $\Lambda$, $\Xi$, $\Omega$ and > their anti-particles produced at mid-rapidity in $Au+Au$ collisions at > RHIC at $\sqrt{s_{NN}}$ = 200 GeV. The yield of multi-strange baryons > per participant nucleon increases from peripheral to central > collisions more rapidly than the $\Lambda$ yield, which appears to > correspond to an increasing strange quark density of matter produced. > The value of the strange phase space occupancy factor $\gamma_{s}$, > obtained from a thermal model fit to the data, approaches unity for the > most central collisions. We also show that the nuclear modification > factors, $R_{CP}$, of $\Lambda$ and $\Xi$ are consistent with each > other and with that of protons in the transverse momentum range 2.0 $< > p_T <$ 5.0 GeV/c. This scaling behaviour is consistent with a scenario > of hadron formation from constituent quark degrees of freedom through > quark recombination or coalescence. > _______________________________________________ Brahms-l mailing list Brahms-l@lists.bnl.gov http://lists.bnl.gov/mailman/listinfo/brahms-lReceived on Thu May 11 09:07:46 2006
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