Re: width of dnd/deta

From: Trine S. Tveter (trine@lynx.uio.no)
Date: Mon Nov 26 2001 - 11:25:17 EST

  • Next message: Jens Jørgen Gaardhøje: "Re: width of dnd/deta"

    Dear Michael and others,
    
    On Mon, 26 Nov 2001, Michael Murray wrote:
    
    > I think it is worth discussing the 
    > change of shape with centrality even if it only reflects the
    > growth of hard collisions at central rapidity. What is |eta| RMS for pp and and
    > what is the reference?
    
    I calculated the width for pp data (UA5, pp at sqrt(s) = 200 GeV - 
    G.J. Alner et al., Z. Phys 33, 1 (1986).) The numbers were read from
    their figure 1 a).  Result: RMS_pp = 2.36+-0.03, which compared to our 
    data is between the RMS values for central and peripheral collisions.  
    The pp point is plotted as a purple circle in the upper panel of
    the figure:
    
    http://lynx.uio.no/trine/brahms/mult/RMS_with_pp_AMPT.gif
    
    together with our sets of RMS values for 200 (red) and 130 (blue) GeV,
    going from central to peripheral collisions from left to right.
    The error bars on the pp point includes (approximately) inaccuracy
    in reading from the figure.
    
    In the lowermost panel of the figure, the pp dN/dEta (purple) and our 
    dN/dEta/(Npart/2) distribution for 0-5% (red) and 40-50% central (blue) 
    collisions are compared. 
    
    I made a similar calculation for the AMPT calculations at 200 GeV,
    taking the numbers from AMPT_xx_xx.dat files in the kansas account.
    The RMS values (calculated over the same Eta interval as for the
    experimental data) follow the experimental points very closely,
    (green points in the upper panel - on top of the red ones.)
    
    Our Figure 4 indicates that the widths as a function of centrality
    evolve differently from 130 to 200 GeV for experimental and
    theoretical results.  I think the theoretical RMS values for 130 GeV
    will vary less with centrality than the experimental ones.  Are the 
    Kharzeev & Levin and AMPT dN/dEta numbers at 130 GeV explicitly 
    available somewhere?  It might be interesting to calculate the 
    theoretical RMS values to find out more about possible interpretations.  
    
    > We may also want to reference to SPS distributions.
    
    Do we have any good SPS references covering a large enough region in Eta
    and where it's possible to compare different centralities (Dieter?)
    
                                           Best wishes,
                                              Trine
    



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