Nuclear stopping in Au + Au collisions at √S NN = 200 GeV

I. G. Bearden, D. Beavis, C. Besliu, B. Budick, H. Bøggild, C. Chasman, C. H. Christensen, P. Christiansen, J. Cibor, R. Debbe, E. Enger, J. J. Gaardhøje, M. Germinario, K. Hagel, O. Hansen, A. Holm, A. K. Holme, H. Ito, A. Jipa, F. JundtJ. I. Jørdre, C. E. Jørgensen, R. Karabowicz, E. J. Kim, T. Kozik, T. M. Larsen, J. H. Lee, Y. K. Lee, G. Løvhøiden, Z. Majka, A. Makeev, M. Mikelsen, M. Murray, J. Natowitz, B. S. Nielsen, J. Norris, K. Olchanski, D. Ouerdane, R. Płaneta, F. Rami, C. Ristea, D. Röhrich, B. H. Samset, D. Sandberg, S. J. Sanders, R. A. Scheetz, P. Staszel, T. S. Tveter, F. Videbæk, R. Wada, Z. Yin, I. S. Zgura

    Research output: Contribution to journalArticlepeer-review


    The proton and antiproton production and baryon stopping in Au + Au collisions at √S NN = 200 GeV were measured. The collision centrality was determined using a multiplicity array located around the nominal interaction point (IP). The net-proton distribution showed that collisions at relativistic heavy ion collider (RHIC) energies were quite transparent compared to lower energies. It was found that the rapidity loss scaling observed at lower energy was broken and the rapidity loss was found to saturate between super proton synchrotron (SPS) and RHIC energies.

    Original languageEnglish (US)
    Article number102301
    Pages (from-to)102301-1-102301-5
    JournalPhysical Review Letters
    Issue number10
    StatePublished - Sep 3 2004

    ASJC Scopus subject areas

    • General Physics and Astronomy


    Dive into the research topics of 'Nuclear stopping in Au + Au collisions at √S NN = 200 GeV'. Together they form a unique fingerprint.

    Cite this