Abstract
Elliptic flow holds much promise for studying the early-time thermalization attained in ultrarelativistic nuclear collisions. Flow measurements also provide a means of distinguishing between hydrodynamic models and calculations which approach the low density (dilute gas) limit. Among the effects that can complicate the interpretation of elliptic flow measurements are azimuthal correlations that are unrelated to the reaction plane (nonflow correlations). Using data for Au + Au collisions at [Formula Presented] from the STAR time projection chamber, it is found that four-particle correlation analyses can reliably separate flow and nonflow correlation signals. The latter account for on average about 15% of the observed second-harmonic azimuthal correlation, with the largest relative contribution for the most peripheral and the most central collisions. The results are also corrected for the effect of flow variations within centrality bins. This effect is negligible for all but the most central bin, where the correction to the elliptic flow is about a factor of 2. A simple new method for two-particle flow analysis based on scalar products is described. An analysis based on the distribution of the magnitude of the flow vector is also described.
Original language | English |
---|---|
Journal | Physical Review C - Nuclear Physics |
Volume | 66 |
Issue number | 3 |
DOIs | |
State | Published - 2002 |
Externally published | Yes |
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In: Physical Review C - Nuclear Physics, Vol. 66, No. 3, 2002.
Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - Elliptic flow from two- and four-particle correlations in Au+Au collisions at [Formula Presented]
AU - Adler, C.
AU - Ahammed, Z.
AU - Allgower, C.
AU - Amonett, J.
AU - Anderson, B. D.
AU - Anderson, M.
AU - Averichev, G. S.
AU - Balewski, J.
AU - Barannikova, O.
AU - Barnby, L. S.
AU - Baudot, J.
AU - Bekele, S.
AU - Belaga, V. V.
AU - Bellwied, R.
AU - Berger, J.
AU - Bichsel, H.
AU - Billmeier, A.
AU - Bland, L. C.
AU - Blyth, C. O.
AU - Bonner, B. E.
AU - Boucham, A.
AU - Brandin, A.
AU - Bravar, A.
AU - Cadman, R. V.
AU - Caines, H.
AU - la Barca Sánchez, M. Calderón
AU - Cardenas, A.
AU - Carroll, J.
AU - Castillo, J.
AU - Castro, M.
AU - Cebra, D.
AU - Chaloupka, P.
AU - Chattopadhyay, S.
AU - Chen, Y.
AU - Chernenko, S. P.
AU - Cherney, M.
AU - Chikanian, A.
AU - Choi, B.
AU - Christie, W.
AU - Coffin, J. P.
AU - Cormier, T. M.
AU - Cramer, J. G.
AU - Crawford, H. J.
AU - Deng, W. S.
AU - Derevschikov, A. A.
AU - Didenko, L.
AU - Dietel, T.
AU - Draper, J. E.
AU - Dunin, V. B.
AU - Dunlop, J. C.
AU - Eckardt, V.
AU - Efimov, L. G.
AU - Emelianov, V.
AU - Engelage, J.
AU - Eppley, G.
AU - Erazmus, B.
AU - Fachini, P.
AU - Faine, V.
AU - Filimonov, K.
AU - Finch, E.
AU - Fisyak, Y.
AU - Flierl, D.
AU - Foley, K. J.
AU - Fu, J.
AU - Gagliardi, C. A.
AU - Gagunashvili, N.
AU - Gans, J.
AU - Gaudichet, L.
AU - Germain, M.
AU - Geurts, F.
AU - Ghazikhanian, V.
AU - Grachov, O.
AU - Grigoriev, V.
AU - Guedon, M.
AU - Gushin, E.
AU - Hallman, T. J.
AU - Hardtke, D.
AU - Harris, J. W.
AU - Henry, T. W.
AU - Heppelmann, S.
AU - Herston, T.
AU - Hippolyte, B.
AU - Hirsch, A.
AU - Hjort, E.
AU - Hoffmann, G. W.
AU - Horsley, M.
AU - Huang, H. Z.
AU - Humanic, T. J.
AU - Igo, G.
AU - Ishihara, A.
AU - Ivanshin, Yu I.
AU - Jacobs, P.
AU - Jacobs, W. W.
AU - Janik, M.
AU - Johnson, I.
AU - Jones, P. G.
AU - Judd, E. G.
AU - Kaneta, M.
AU - Kaplan, M.
AU - Keane, D.
AU - Kiryluk, J.
AU - Kisiel, A.
AU - Klay, J.
AU - Klein, S. R.
AU - Klyachko, A.
AU - Konstantinov, A. S.
AU - Kopytine, M.
AU - Kotchenda, L.
AU - Kovalenko, A. D.
AU - Kramer, M.
AU - Kravtsov, P.
AU - Krueger, K.
AU - Kuhn, C.
AU - Kulikov, A. I.
AU - Kunde, G. J.
AU - Kunz, C. L.
AU - Kutuev, R. Kh
AU - Kuznetsov, A. A.
AU - Lakehal-Ayat, L.
AU - Lamont, M. A.C.
AU - Landgraf, J. M.
AU - Lange, S.
AU - Lansdell, C. P.
AU - Lasiuk, B.
AU - Laue, F.
AU - Lebedev, A.
AU - Lednický, R.
AU - Leontiev, V. M.
AU - LeVine, M. J.
AU - Li, Q.
AU - Lindenbaum, S. J.
AU - Lisa, M. A.
AU - Liu, F.
AU - Liu, L.
AU - Liu, Z.
AU - Liu, Q. J.
AU - Ljubicic, T.
AU - Llope, W. J.
AU - LoCurto, G.
AU - Long, H.
AU - Longacre, R. S.
AU - Lopez-Noriega, M.
AU - Love, W. A.
AU - Ludlam, T.
AU - Lynn, D.
AU - Ma, J.
AU - Majka, R.
AU - Margetis, S.
AU - Markert, C.
AU - Martin, L.
AU - Marx, J.
AU - Matis, H. S.
AU - Matulenko, Yu A.
AU - McShane, T. S.
AU - Meissner, F.
AU - Melnick, Yu
AU - Meschanin, A.
AU - Messer, M.
AU - Miller, M. L.
AU - Milosevich, Z.
AU - Minaev, N. G.
AU - Mitchell, J.
AU - Moiseenko, V. A.
AU - Moore, C. F.
AU - Morozov, V.
AU - Moura, M. M.
AU - Munhoz, M. G.
AU - Nelson, J. M.
AU - Nevski, P.
AU - Nikitin, V. A.
AU - Nogach, L. V.
AU - Norman, B.
AU - Nurushev, S. B.
AU - Odyniec, G.
AU - Ogawa, A.
AU - Okorokov, V.
AU - Oldenburg, M.
AU - Olson, D.
AU - Paic, G.
AU - Pandey, S. U.
AU - Panebratsev, Y.
AU - Panitkin, S. Y.
AU - Pavlinov, A. I.
AU - Pawlak, T.
AU - Perevoztchikov, V.
AU - Peryt, W.
AU - Petrov, V. A.
AU - Planinic, M.
AU - Pluta, J.
AU - Porile, N.
AU - Porter, J.
AU - Poskanzer, A. M.
AU - Potrebenikova, E.
AU - Prindle, D.
AU - Pruneau, C.
AU - Putschke, J.
AU - Rai, G.
AU - Rakness, G.
AU - Ravel, O.
AU - Ray, R. L.
AU - Razin, S. V.
AU - Reichhold, D.
AU - Reid, J. G.
AU - Renault, G.
AU - Retiere, F.
AU - Ridiger, A.
AU - Ritter, H. G.
AU - Roberts, J. B.
AU - Rogachevski, O. V.
AU - Romero, J. L.
AU - Rose, A.
AU - Roy, C.
AU - Rykov, V.
AU - Sakrejda, I.
AU - Salur, S.
AU - Sandweiss, J.
AU - Saulys, A. C.
AU - Savin, I.
AU - Schambach, J.
AU - Scharenberg, R. P.
AU - Schmitz, N.
AU - Schroeder, L. S.
AU - Schüttauf, A.
AU - Schweda, K.
AU - Seger, J.
AU - Seliverstov, D.
AU - Seyboth, P.
AU - Shahaliev, E.
AU - Shestermanov, K. E.
AU - Shimanskii, S. S.
AU - Shvetcov, V. S.
AU - Skoro, G.
AU - Smirnov, N.
AU - Snellings, R.
AU - Sorensen, P.
AU - Sowinski, J.
AU - Spinka, H. M.
AU - Srivastava, B.
AU - Stephenson, E. J.
AU - Stock, R.
AU - Stolpovsky, A.
AU - Strikhanov, M.
AU - Stringfellow, B.
AU - Struck, C.
AU - Suaide, A. A.P.
AU - Sugarbaker, E.
AU - Suire, C.
AU - Šumbera, M.
AU - Surrow, B.
AU - Symons, T. J.M.
AU - Szanto de Toledo, A.
AU - Szarwas, P.
AU - Tai, A.
AU - Takahashi, J.
AU - Tang, A. H.
AU - Thomas, J. H.
AU - Thompson, M.
AU - Tikhomirov, V.
AU - Tokarev, M.
AU - Tonjes, M. B.
AU - Trainor, T. A.
AU - Trentalange, S.
AU - Tribble, R. E.
AU - Trofimov, V.
AU - Tsai, O.
AU - Ullrich, T.
AU - Underwood, D. G.
AU - Van Buren, G.
AU - VanderMolen, A. M.
AU - Vasilevski, I. M.
AU - Vasiliev, A. N.
AU - Vigdor, S. E.
AU - Voloshin, S. A.
AU - Wang, F.
AU - Ward, H.
AU - Watson, J. W.
AU - Wells, R.
AU - Westfall, G. D.
AU - Whitten, C.
AU - Wieman, H.
AU - Willson, R.
AU - Wissink, S. W.
AU - Witt, R.
AU - Wood, J.
AU - Xu, N.
AU - Xu, Z.
AU - Yakutin, A. E.
AU - Yamamoto, E.
AU - Yang, J.
AU - Yepes, P.
AU - Yurevich, V. I.
AU - Zanevski, Y. V.
AU - Zborovský, I.
AU - Zhang, H.
AU - Zhang, W. M.
AU - Zoulkarneev, R.
AU - Zubarev, A. N.
PY - 2002
Y1 - 2002
N2 - Elliptic flow holds much promise for studying the early-time thermalization attained in ultrarelativistic nuclear collisions. Flow measurements also provide a means of distinguishing between hydrodynamic models and calculations which approach the low density (dilute gas) limit. Among the effects that can complicate the interpretation of elliptic flow measurements are azimuthal correlations that are unrelated to the reaction plane (nonflow correlations). Using data for Au + Au collisions at [Formula Presented] from the STAR time projection chamber, it is found that four-particle correlation analyses can reliably separate flow and nonflow correlation signals. The latter account for on average about 15% of the observed second-harmonic azimuthal correlation, with the largest relative contribution for the most peripheral and the most central collisions. The results are also corrected for the effect of flow variations within centrality bins. This effect is negligible for all but the most central bin, where the correction to the elliptic flow is about a factor of 2. A simple new method for two-particle flow analysis based on scalar products is described. An analysis based on the distribution of the magnitude of the flow vector is also described.
AB - Elliptic flow holds much promise for studying the early-time thermalization attained in ultrarelativistic nuclear collisions. Flow measurements also provide a means of distinguishing between hydrodynamic models and calculations which approach the low density (dilute gas) limit. Among the effects that can complicate the interpretation of elliptic flow measurements are azimuthal correlations that are unrelated to the reaction plane (nonflow correlations). Using data for Au + Au collisions at [Formula Presented] from the STAR time projection chamber, it is found that four-particle correlation analyses can reliably separate flow and nonflow correlation signals. The latter account for on average about 15% of the observed second-harmonic azimuthal correlation, with the largest relative contribution for the most peripheral and the most central collisions. The results are also corrected for the effect of flow variations within centrality bins. This effect is negligible for all but the most central bin, where the correction to the elliptic flow is about a factor of 2. A simple new method for two-particle flow analysis based on scalar products is described. An analysis based on the distribution of the magnitude of the flow vector is also described.
UR - http://www.scopus.com/inward/record.url?scp=84872911566&partnerID=8YFLogxK
U2 - 10.1103/PhysRevC.66.034904
DO - 10.1103/PhysRevC.66.034904
M3 - Article
AN - SCOPUS:84872911566
SN - 0556-2813
VL - 66
JO - Physical Review C - Nuclear Physics
JF - Physical Review C - Nuclear Physics
IS - 3
ER -