Fw: Release of STAR 200 GeV Spectra Paper

From: Flemming Videbaek (videbaek@rcf.rhic.bnl.gov)
Date: Thu Sep 25 2003 - 08:45:20 EDT

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    FYI
    ------------------------------------------------------
    Flemming Videbaek
    Physics Department
    Brookhaven National Laboratory
    
    tlf: 631-344-4106
    fax 631-344-1334
    e-mail: videbaek@bnl.gov
    
    ----- Original Message ----- 
    From: "Timothy Hallman" <hallman@bnl.gov>
    To: <tkirk@bnl.gov>; <zajc@nevis.columbia.edu>; <videbaek@bnl.gov>; <gunther.roland@cern.ch>
    Cc: <hallman@bnl.gov>
    Sent: Wednesday, September 24, 2003 10:13 PM
    Subject: Release of STAR 200 GeV Spectra Paper
    
    
    | Dear Tom, Bill, Flemming, and Gunther,
    |
    | I am pleased to announce STAR's intention to submit a new
    | paper on "Identified particle distributions in pp and AuAu
    | collisions roots_NN = 200 GeV" to Physical Review Letters
    | one week from today. The title and abstract for the paper
    | are enclosed.
    |
    |                      Sincerely,
    |
    |                       Tim
    |
    |
    |
    | "Identified particle distributions in pp and AuAu
    | collisions roots_NN = 200 GeV"
    |
    | Transverse mass and rapidity distributions for charged pions,
    | charged kaons, protons, and antiprotons are reported for
    | roots_NN = 200 GeV pp and Au+Au collisions at RHIC. The
    | transverse mass distributions are rapidity independent within
    | |y| < 0.5, consistent with a boost ­invariant system in this
    | rapidity interval. Spectral shapes and relative particle yields
    | are similar in pp and peripheral Au+Au collisions and change
    | smoothly to central Au+Au collisions. No centrality dependence
    | was observed in the kaon and antiproton production rates relative
    | to the pion production rate from medium­ central to central
    | collisions. Chemical and kinetic equilibrium model fits to
    | our data reveal strong radial flow and relatively long duration
    | from chemical to kinetic freezeout in central Au+Au collisions.
    | The chemical freeze-out temperature appears to be independent
    | of initial conditions at RHIC energies.
    |
    


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