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Strangeness in Au+Au collisions at √sNN = 130 GeV observed with the STAR detector

  • L. S. Barnby
  • , C. Adler
  • , Z. Ahammed
  • , C. Allgower
  • , J. Amonett
  • , B. D. Anderson
  • , M. Anderson
  • , G. S. Averichev
  • , J. Balewski
  • , O. Barannikova
  • , J. Baudot
  • , S. Bekele
  • , V. V. Belaga
  • , R. Bellwied
  • , J. Berger
  • , H. Bichsel
  • , L. C. Bland
  • , C. O. Blyth
  • , B. E. Bonner
  • , A. Boucham
  • A. Brandin, R. V. Cadman, H. Caines, M. de la Calderón Barca Sánchez, A. Cardenas, J. Carroll, J. Castillo, M. Castro, D. Cebra, S. Chattopadhyay, M. L. Chen, Y. Chen, S. P. Chernenko, M. Cherney, A. Chikanian, B. Choi, W. Christie, J. P. Coffin, T. M. Cormier, J. G. Cramer, H. J. Crawford, W. S. Deng, A. A. Derevschikov, L. Didenko, J. E. Draper, V. B. Dunin, J. C. Dunlop, V. Eckardt, L. G. Efimov, V. Emelianov, J. Engelage, G. Eppley, B. Erazmus, P. Fachini, V. Faine, K. Filimonov, E. Finch, Y. Fisyak, D. Flierl, K. J. Foley, J. Fu, C. A. Gagliardi, N. Gagunashvili, J. Gans, L. Gaudichet, M. Germain, F. Geurts, V. Ghazikhanian, J. Grabski, O. Grachov, V. Grigoriev, M. Guedon, E. Gushin, T. J. Hallman, D. Hardtke, J. W. Harris, M. Heffner, S. Heppelmann, T. Herston, B. Hippolyte, A. Hirsch, E. Hjort, G. W. Hoffmann, M. Horsley, H. Z. Huang, T. J. Humanic, H. Hümmler, G. Igo, A. Ishihara, Y. I. Ivanshin, P. Jacobs, W. W. Jacobs, M. Janik, I. Johnson, P. G. Jones, E. G. Judd, M. Kaneta, M. Kaplan, D. Keane, J. Kiryluk, A. Kisiel, J. Klay, S. R. Klein, A. Klyachko, A. S. Konstantinov, L. Kotchenda, A. D. Kovalenko, M. Kramer, P. Kravtsov, K. Krueger, C. Kuhn, A. I. Kulikov, G. J. Kunde, C. L. Kunz, R. K. Kutuev, A. A. Kuznetsov, L. Lakehal-Ayat, M. A.C. Lamont, J. M. Landgraf, S. Lange, C. P. Lansdell, B. Lasiuk, F. Laue, A. Lebedev, R. Lednický, V. M. Leontiev, M. J. LeVine, Q. Li, S. J. Lindenbaum, M. A. Lisa, F. Liu, L. Liu, Z. Liu, Q. J. Liu, T. Ljubicic, W. J. Llope, G. lo Curto, H. Long, R. S. Longacre, M. Lopez-Noriega, W. A. Love, D. Lynn, R. Majka, S. Margetis, C. Markert, L. Martin, J. Marx, H. S. Matis, Y. A. Matulenko, T. S. McShane, F. Meissner, Y. Melnick, A. Meschanin, M. Messer, M. L. Miller, Z. Milosevich, N. G. Minaev, J. Mitchell, V. A. Moiseenko, C. F. Moore, V. Morozov, M. M. de Moura, M. G. Munhoz, J. M. Nelson, P. Nevski, V. A. Nikitin, L. V. Nogach, B. Norman, S. B. Nurushev, G. Odyniec, A. Ogawa, V. Okorokov, M. Oldenburg, D. Olson, G. Paic, S. U. Pandey, Y. Panebratsev, S. Y. Panitkin, A. I. Pavlinov, T. Pawlak, V. Perevoztchikov, W. Peryt, V. A. Petrov, J. Pluta, N. Porile, J. Porter, A. M. Poskanzer, E. Potrebenikova, D. Prindle, C. Pruneau, S. Radomski, G. Rai, O. Ravel, R. L. Ray, S. V. Razin, D. Reichhold, J. G. Reid, F. Retiere, A. Ridiger, H. G. Ritter, J. B. Roberts, O. V. Rogachevski, J. L. Romero, C. Roy, V. Rykov, I. Sakrejda, J. Sandweiss, A. C. Saulys, I. Savin, J. Schambach, R. P. Scharenberg, N. Schmitz, L. S. Schroeder, A. Schüttauf, K. Schweda, J. Seger, D. Seliverstov, P. Seyboth, E. Shahaliev, K. E. Shestermanov, S. S. Shimanskii, V. S. Shvetcov, G. Skoro, N. Smirnov, R. Snellings, P. Sorensen, J. Sowinski, H. M. Spinka, B. Srivastava, E. J. Stephenson, R. Stock, A. Stolpovsky, M. Strikhanov, B. Stringfellow, C. Struck, A. A.P. Suaide, E. Sugarbaker, C. Suire, M. Šumbera, T. J.M. Symons, A. Szanto de Toledo, P. Szarwas, A. Tai, J. Takahashi, A. H. Tang, J. H. Thomas, M. Thompson, V. Tikhomirov, M. Tokarev, M. B. Tonjes, T. A. Trainor, S. Trentalange, R. E. Tribble, V. Trofimov, O. Tsai, K. Turner, T. Ullrich, D. G. Underwood, G. van Buren, A. M. van der Molen, I. M. Vasilevski, A. N. Vasiliev, S. E. Vigdor, S. A. Voloshin, F. Wang, H. Ward, J. W. Watson, R. Wells, T. Wenaus, G. D. Westfall, C. Whitten, H. Wieman, R. Willson, S. W. Wissink, R. Witt, J. Wood, N. Xu, Z. Xu, A. E. Yakutin, E. Yamamoto, J. Yang, P. Yepes, V. I. Yurevich, Y. V. Zanevski, I. Zborovský, H. Zhang, W. M. Zhang, R. Zoulkarneev, A. N. Zubarev
  • Kent State University
  • Goethe University Frankfurt
  • Purdue University
  • Indiana University Bloomington
  • University of California at Davis
  • Joint Institute for Nuclear Research
  • Institut de Recherches Subatomiques
  • Ohio State University
  • Wayne State University
  • University of Washington
  • University of Birmingham
  • Rice University
  • SUBATECH
  • Moscow Engineering Physics Institute
  • Argonne National Laboratory
  • Yale University
  • Lawrence Berkeley National Laboratory
  • Brookhaven National Laboratory
  • University of California at Los Angeles
  • Creighton University
  • University of Texas at Austin
  • University of California at Berkeley
  • Institute for High Energy Physics
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • Universidade de São Paulo
  • Texas A&M University
  • Warsaw University of Technology
  • Pennsylvania State University
  • Carnegie Mellon University
  • City University of New York
  • Central China Normal University
  • Michigan State University

Research output: Contribution to journalArticlepeer-review

11 Scopus citations

Abstract

The STAR detector has made a variety of measurements of strange and other hadronic species in Au+Au collisions at √sNN = 130 GeV. A comparison of kaon and pion production enables an examination of the systematics of strangers production with energy by comparing them to lower energy collisions. Anti-baryon to baryon ratios indicate a much reduced net-baryon density and transverse momentum spectra show that a picture of transverse expansion seems appropriate.

Original languageEnglish
Article number303
Pages (from-to)1535-1542
Number of pages8
JournalJournal of Physics G: Nuclear and Particle Physics
Volume28
Issue number7
DOIs
StatePublished - Jul 2002

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