follow-up on previous e-mail /fv ---------------------------------------------------------------- Flemming Videbaek Physics Department Brookhaven National Laboratory e-mail: videbaek@bnl.gov phone: 631-344-4106 ----- Original Message ----- From: <Boris.Kopeliovich@mpi-hd.mpg.de> To: "Dmitri Kharzeev" <kharzeev@bnl.gov> Cc: "Dmitri E Kharzeev" <kharzeev@quark.phy.bnl.gov>; "Yuri Kovchegov" <yuri@qcd.phys.washington.edu>; "Mikkel B. Johnson" <mbjohnson@lanl.gov>; "Hans-Juergen Pirner" <pir@tphys.uni-heidelberg.de>; "Kirill Tuchin" <tuchin@quark.phy.bnl.gov>; "Alfred Mueller" <arb@phys.columbia.edu>; "Ivan Schmidt" <ivan.schmidt@usm.cl>; "Larry McLerran" <mclerran@quark.phy.bnl.gov>; "flemming videbaek" <videbaek@rcf.rhic.bnl.gov> Sent: Tuesday, March 15, 2005 6:26 PM Subject: Re: pt spectra from h-h, h-A and A-A at SPS (NA49 data) (fwd) > Hi Dima, > thanks for the quick response. Let me comment on it. > > > The data you sent us extend to p_t less than 2 GeV, which is still below > > the Cronin peak. The data thus do not tell anything about the > > disappearance of the Cronin peak, and especially about the behavior > > above p_t's at which the peak is normally located. > > I don't think that it is specifically important whether the Cronin maximum > is above or below one. It might be even still above one, since the effect > is much stronger at SPS than at RHIC. Important is that the effect of > suppression at large xF is not only a property of soft, low pT, production > (what has been known for decades), but spans across large a pT interval. > You can see that the amount of suppression hardly depends on pT, as we > expected. I think it is a challenge to find an explanation alternative to > ours. > > > Moreover, there is a very important difference between the physics at > > the NA49 energy of about 20 GeV (cms) and RHIC energy of 200 GeV, as it > > is nicely illustrated for example in the article by Bourrely and Soffer, > > hep-ph/0311110. > > > > As can be seen in Figs 2-5 of that paper, and in many calculations done > > by Werner Vogelsang, NLO pQCD does a beautiful job in explaining the > > pion p_t spectra at mid- and forward rapidities at RHIC energy. However, > > these calculations fail miserably in describing the spectra at 20 GeV, > > even at mid-rapidity. This shows very clearly that non-perturbative > > phenomena dominate at 20 GeV, but the perturbative description of pp > > interactions begins to apply at RHIC energy of 200 GeV. > > No mystery, this is exactly what our paper is about: not the perturbative > QCD, but factorization breaks down when one approaches the kinematic > limit. And you can see this in all the figures you mentioned from the > Bourrely and Soffer paper. For instance, Fig.2 demonstrates that > factorization works at xF=0 and medium-high pT, but then fails, and more > at lower energies. Of course, one can move towards the kinematic limit > increasing either xF, or pT. I don't know why you call this > nonperturbative effects, according to our paper this is just due to > problems with sharing energy withing high Fock components. > > > > > > It is thus unlikely, in my opinion, that the same mechanism is > > responsible for the high p_t suppression observed at RHIC and SPS > > energies. On the experimental side, it seems we still do not know > > whether the high p_t suppression develops around the position of the > > Cronin peak at the SPS energy. > > What should probably convince you is a numerical comparison of our > calculations with the NA49 data. We will do it shortly using the same > mechanism and the same computer code. Will see what comes out. > > All the best, > Boris > _______________________________________________ Brahms-l mailing list Brahms-l@lists.bnl.gov http://lists.bnl.gov/mailman/listinfo/brahms-lReceived on Tue Mar 15 19:02:20 2005
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