Dear Michael, I apologize for my delayed response! In the last days some works at the new network did not permit to answer you. >From Saturday on Sunday night is snowing and I can communicate easily! I observed that Dr.Bearden solved the problem with the pbar symbol in root. The bin was 0.125 rapidity units. The global values of the pbar/p ratios are in text. I will send the other values if you wish! Now we work on the UrQMD prediction, especially on the temporal sequence. Some interesting results appear, as well as some difference form the HIJING predictions for different collision developing times. Some connections with the particle detected in ZDCs are interesting. We will try to compare with the data from the last irradiation month. If you have some spectra in ZDCs (for neutrons, mainly, but for other particles too) we greatly appreciate to receive a few to compare with ours! Sincerely yours, Alexandru -----Original Message----- From: Michael Murray <murray@cyclotronmail.tamu.edu> To: brahms-l@bnl.gov <brahms-l@bnl.gov> Date: Monday, February 19, 2001 8:30 PM Subject: Re: Comments on BRAHMS paper drafts > Dear Alexandru, > thanks for the Hging plots. Could you please tell me >how many bins/unit rapidity. Also could you please make the pbar/p >ratios. Finally how did you manage to make a pbar symbol in root? > Yoours Michael > >Quoting "Al.Jipa" <ajip@scut.fizica.unibuc.ro>: > >> Dear coleagues, >> >> We sent some results on antiproton to proton ratio obtained using >> HIJING >> predictions. I hope that these results will be useful! >> We would like to correct the name of Sorin, namely: Ion Sorin ZGURA >> (previous name was SGURA). >> T.F.Thorsteinsen and Z.Sosin are not BRAHMS members from Bucharest >> University. >> A detailed analysis using the temporal evolution for each collision will >> be >> done soon. >> The first results on multiplicity give values of charged particles, in >> central collisions, between 3200 and 4500. >> Sincerely yours, >> >> Alexandru JIPA, >> Sorin ZGURA, >> Calin BESLIU >> >> -----Original Message----- >> From: Jens Jorgen Gaardhoje <gardhoje@nbi.dk> >> To: brahms-l@bnl.gov <brahms-l@bnl.gov> >> Date: Monday, January 22, 2001 8:30 PM >> Subject: BRAHMS paper drafts (2) >> >> >> Dear BRAHMS friends >> >> AS agreed last week I send you two drafts for upcoming BRAHMS papers >> (MSWord). >> >> I have taken the liberty of including a number of footnotes, where >> things need to be checked and worked on. I have also suggested names >> for >> the various tasks in order to speed up the process. I hope that people >> will get together with their colleagues (also those few that have no >> definite task) and respond quickly. Please send me your comments to >> text >> as well as philosophy. >> >> best regards >> JJ >> >> -- >> ____________________________________________________ >> JENS JORGEN GAARDHOJE >> Assoc. Prof. of Physics, Dr. Scient. >> >> Niels Bohr Institute, >> University of Copenhagen >> Blegdamsvej 17, 2100 Copenhagen >> Denmark. >> >> Tlf: (+45) 35 32 53 09 (dir) >> (+45) 35 32 52 09 (secr) >> Fax: (+45) 35 32 50 16 >> Email: gardhoje @ nbi.dk >> Home page: http://alf.nbi.dk/~gardhoje >> >> -Chair Ph. D. School of Physics at NBI.F.AFG. >> (secr. Frank Kristensen 35 32 04 41, Ørsted Lab.) >> -Member Danish National Commission for UNESCO >> (secr. Ulla Holm 35 32 52 72, NBI) >> ___________________________________________________ >> > > > >Michael Murray, Cyclotron TAMU, 979 845 1411 x 273, Fax 1899 >
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