Three-pion Hanbury Brown-Twiss correlations in relativistic heavy-ion collisions from the STAR experiment.

J. Adams,C. Adler,Z. Ahammed,C. Allgower,J. Amonett,B. Anderson,M. Anderson,D. Arkhipkin,G. S. Averichev,J. Balewski,O. Barannikova,L. Barnby,J. Baudot,S. Bekele,V. Belaga,R. Bellwied,J. Berger,H. Bichsel,A. Billmeier,L. Bland,C. Blyth,B. Bonner,M. Botje,A. Boucham,A. Brandin,A. Bravar,R. Cadman,X. Cai,H. Caines,M. Calderon De La Barca Sanchez,A. Cardenas,J. Carroll,J. Castillo,M. Castro,D. Cebra,P. Chaloupka,S. Chattopadhyay,Y. Chen,S. Chernenko,M. Cherney,A. Chikanian,B. Choi,W. Christie,J. Coffin,T. Cormier,M. Mora Corral,J. Cramer,H. Crawford,A. Derevschikov,L. Didenko,T. Dietel,J. Draper,V. Dunin,J. Dunlop,V. Eckardt,L. Efimov,V. Emelianov,J. Engelage,G. Eppley,B. Erazmus,P. Fachini,V. Faine,J. Faivre,R. Fatemi,K. Filimonov,E. Finch,Y. Fisyak,D. Flierl,K. J. Foley,J. Fu,C. Gagliardi,N. Gagunashvili,J. Gans,L. Gaudichet,M. Germain,F. Geurts,V. Ghazikhanian,Oleg A Grachov,M. Guedon,S. Guertin,E. Gushin,T. Gutierrez,T. Hallman,D. Hardtke,J. Harris,M. Heinz,T. Henry,S. Heppelmann,T. Herston,B. Hippolyte,A. Hirsch,E. Hjort,G. Hoffmann,M. Horsley,H. Huang,T. Humanic,G. Igo,A. Ishihara,P. Jacobs,W. Jacobs,M. Janik,I. Johnson,P. Jones,E. Judd,S. Kabana,M. Kaneta,M. Kaplan,D. Keane,J. Kiryluk,A. Kisiel,J. Klay,S. Klein,A. Klyachko,T. Kollegger,A. Konstantinov,M. Kopytine,L. Kotchenda,A. Kovalenko,M. Kramer,P. Kravtsov,K. Krueger,C. Kuhn,A. Kulikov,G. Kunde,C. Kunz,R. Kutuev,A. Kuznetsov,M. Lamont,J. Landgraf,S. Lange,C. Lansdell,B. Lasiuk,F. Laue,J. Lauret,A. Lebedev,R. Lednický,V. Leontiev,M. Levine,Q. Li,S. Lindenbaum,M. Lisa,F. Liu,L. Liu,Z. Liu,Q. Liu,T. Ljubičić,W. Llope,H. Long,R. Longacre,M. López-Noriega,W. Love,T. Ludlam,D. Lynn,J. Ma,Y. Ma,D. Magestro,R. Majka,S. Margetis,C. Markert,L. Martin,J. Marx,H. Matis,Y. Matulenko,T. McShane,F. Meissner,Y. Melnick,A. Meschanin,M. Messer,M. Miller,Z. Milosevich,N. Minaev,J. Mitchell,L. Molnár,C. F. Moore,V. Morozov,M. M. de Moura,M. Munhoz,J. Nelson,P. Nevski,V. Nikitin,L. Nogach,B. Norman,S. Nurushev,G. Odyniec,A. Ogawa,V. Okorokov,M. Oldenburg,D. Olson,G. Paic,S. Pandey,Y. Panebratsev,S. Panitkin,A. Pavlinov,T. Pawlak,V. Perevoztchikov,W. Peryt,V. Petrov,R. Picha,M. Planinić,J. Pluta,N. Porile,J. Porter,A. Poskanzer,E. Potrebenikova,D. Prindle,C. Pruneau,J. Putschke,G. Rai,G. Rakness,O. Ravel,R. Ray,S. Razin,D. Reichhold,J. Reid,G. Renault,F. Retière,A. Ridiger,H. Ritter,J. Roberts,O. Rogachevski,J. Romero,A. Rose,C. Roy,V. Rykov,I. Sakrejda,S. Salur,J. Sandweiss,I. Savin,J. Schambach,R. Scharenberg,N. Schmitz,L. Schroeder,K. Schweda,J. Seger,P. Seyboth,E. Shahaliev,K. Shestermanov,S. Shimanskii,F. Simon,G. Škoro,N. Smirnov,R. Snellings,P. Sorensen,J. Sowinski,H. Spinka,B. Srivastava,E. Stephenson,R. Stock,A. Stolpovsky,M. Strikhanov,B. Stringfellow,C. Struck,A. Suaide,E. Sugarbaker,C. Suire,M. Šumbera,B. Surrow,T. Symons,A. Szanto de Toledo,P. Szarwas,A. Tai,J. Takahashi,A. Tang,D. Thein,J. Thomas,M. Thompson,S. Timoshenko,M. Tokarev,M. Tonjes,T. Trainor,S. Trentalange,R. Tribble,V. Trofimov,O. Tsai,T. Ullrich,D. Underwood,G. Van Buren,A. Vander Molen,A. Vasiliev,S. Vigdor,S. Voloshin,M. Vznuzdaev,F. Wang,Y. Wang,H. Ward,J. Watson,R. Wells,G. Westfall,C. Whitten,H. Wieman,R. Willson,S. Wissink,R. Witt,J. Wood,N. Xu,Z. Xu,A. Yakutin,E. Yamamoto,J. Yang,P. Yepes,V. Yurevich,Y. Zanevski,I. Zborovský,H. Zhang,W. Zhang,R. Zoulkarneev,J. Zoulkarneeva,A. Zubarev

Published 2003 in Physical Review Letters

ABSTRACT

Data from the first physics run at the Relativistic Heavy-Ion Collider at Brookhaven National Laboratory, Au+Au collisions at sqrt[s(NN)]=130 GeV, have been analyzed by the STAR Collaboration using three-pion correlations with charged pions to study whether pions are emitted independently at freeze-out. We have made a high-statistics measurement of the three-pion correlation function and calculated the normalized three-particle correlator to obtain a quantitative measurement of the degree of chaoticity of the pion source. It is found that the degree of chaoticity seems to increase with increasing particle multiplicity.

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