Charged Kaon Interferometric Probes Of Space-Time Evolution In Au Plus Au Collisions At S(Nn)=200 Gev

S. Afanasiev, C. Aidala,N. Ajitanand,Y. Akiba,J. Alexander,A. Al-Jamel,K. Aoki,L. Aphecetche,R. Armendariz,S. Aronson,R. Averbeck,T. Awes,B. Azmoun,V. Babintsev, A. Baldisseri,K. Barish,P. Barnes,B. Bassalleck,S. Bathe,S. Batsouli,V. Baublis,F. Bauer, A. Bazilevsky,S. Belikov,R. Bennett,Y. Berdnikov,M. Bjorndal,J. Boissevain,H. Borel,K. Boyle,M. Brooks,D. Brown,D. Bucher,H. Buesching,V. Bumazhnov,G. Bunce,J. Burward-Hoy,S. Butsyk,S. Campbell,J.-S. Chai,S. Chernichenko,J. Chiba,C. Chi,M. Chiu,I. Choi, T. Chujo,V. Cianciolo,C. Cleven,Y. Cobigo,B. Cole,M. Comets,P. Constantin,M. Csanád,T. Csörgő,T. Dahms,K. Das,G. David,H. Delagrange,A. Denisov,D. d’Enterria,A. Deshpande,E. Desmond,O. Dietzsch,A. Dion,J. Drachenberg,O. Drapier,A. Drees,A. Dubey,A. Durum,V. Dzhordzhadze,Y. Efremenko,J. Egdemir,A. Enokizono,H. En’yo,B. Espagnon, S. Esumi,D. Fields,F. Fleuret,S. Fokin,B. Forestier, Z. Fraenkel,J. Frantz,A. Franz,A. Frawley,Y. Fukao,S.-Y. Fung,S. Gadrat,F. Gastineau,M. Germain,A. Glenn, M. Gonin,J. Gosset,Y. Goto,R. Granier de Cassagnac, N. Grau,S. Greene,M. Grosse Perdekamp,T. Gunji,H.-Å. Gustafsson,T. Hachiya,A. Hadj Henni,J. Haggerty,M. Hagiwara, H. Hamagaki,H. Harada,E. Hartouni,K. Haruna,M. Harvey,E. Haslum,K. Hasuko,R. Hayano,M. Heffner,T. Hemmick,J. Heuser,X. He,H. Hiejima,J. Hill,R. Hobbs,M. Holmes,W. Holzmann,K. Homma,B. Hong,T. Horaguchi,M. Hur,T. Ichihara,K. Imai,M. Inaba,D. Isenhower,L. Isenhower,M. Ishihara,T. Isobe,M. Issah,A. Isupov,B. Jacak, J. Jia,J. Jin, O. Jinnouchi,B. Johnson,K. Joo,D. Jouan,F. Kajihara,S. Kametani,N. Kamihara,M. Kaneta,J. Kang,T. Kawagishi,A. Kazantsev,S. Kelly,A. Khanzadeev,D. Kim,E. Kim,Y.-S. Kim, E. Kinney,Á. Kiss,E. Kistenev,A. Kiyomichi,C. Klein-Boesing,L. Kochenda,V. Kochetkov,B. Komkov,M. Konno,D. Kotchetkov, A. Kozlov,P. Kroon,G. Kunde,N. Kurihara,K. Kurita,M. Kweon,Y. Kwon,G. Kyle,R. Lacey,J. Lajoie, A. Lebedev,Y. Le Bornec,S. Leckey,D. Lee,M. Lee,M. Leitch,M. Leite,H. Lim,A. Litvinenko,M. Liu,X. Li, C. Maguire,Y. Makdisi,A. Malakhov,M. Malik,V. Manko,H. Masui,F. Matathias,M. McCain,P. McGaughey, Y. Miake,T. Miller,A. Milov,S. Mioduszewski,G. Mishra,J. Mitchell,D. Morrison,J. Moss,T. Moukhanova,D. Mukhopadhyay,J. Murata,S. Nagamiya, Y. Nagata,J. Nagle,M. Naglis,T. Nakamura,J. Newby,M. Nguyen,B. Norman,R. Nouicer,A. Nyanin, J. Nystrand,E. O’Brien,C. Ogilvie,H. Ohnishi,I. Ojha,H. Okada, K. Okada,O. Omiwade, A. Oskarsson,I. Otterlund,K. Ozawa,D. Pal,A. Palounek,V. Pantuev, V. Papavassiliou,J. Park, W. Park,S. Pate,H. Pei,J.-C. Peng,H. Pereira,V. Peresedov,D. Peressounko,C. Pinkenburg,R. Pisani,M. Purschke, A. Purwar,H. Qu,J. Rak,I. Ravinovich,K. Read,M. Reuter,K. Reygers,V. Riabov,Y. Riabov, G. Roche,A. Romana,M. Rosati, S. Rosendahl, P. Rosnet,P. Rukoyatkin,V. Rykov,S. Ryu,B. Sahlmueller,N. Saito,T. Sakaguchi,S. Sakai,V. Samsonov,H. Sato,S. Sato,S. Sawada,V. Semenov, R. Seto,D. Sharma,T. Shea,I. Shein,T.-A. Shibata,K. Shigaki,M. Shimomura,T. Shohjoh,K. Shoji,A. Sickles,C. Silva, D. Silvermyr,K. Sim,C. Singh,V. Singh,S. Skutnik,W. Smith,A. Soldatov,R. Soltz,W. Sondheim,S. Sorensen,I. Sourikova,F. Staley,P. Stankus, E. Stenlund,M. Stepanov,A. Ster,S. Stoll, T. Sugitate, C. Suire,J. Sullivan,J. Sziklai,T. Tabaru,S. Takagi,E. Takagui,A. Taketani, K. Tanaka,Y. Tanaka,K. Tanida,M. Tannenbaum,A. Taranenko,P. Tarján,T. Thomas,M. Togawa, J. Tojo,H. Torii,R. Towell,V. N. Tram,I. Tserruya,Y. Tsuchimoto,S. Tuli,H. Tydesjö, N. Tyurin,C. Vale,H. Valle,H. van Hecke, J. Velkovska,R. Vértesi, A. Vinogradov,E. Vznuzdaev,M. Wagner,X. Wang,Y. Watanabe,J. Wessels,S. White,N. Willis,D. Winter,C. Woody,M. Wysocki, W. Xie,A. Yanovich,S. Yokkaichi,G. Young,I. Younus,I. Yushmanov,W. Zajc,O. Zaudtke,C. Zhang,J. Zimányi,L. Zolin

PHYSICAL REVIEW LETTERS(2009)

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摘要
Bose-Einstein correlations of charged kaons are used to probe Au+Au collisions at s(NN)=200 GeV and are compared to charged pion probes, which have a larger hadronic scattering cross section. Three-dimensional Gaussian source radii are extracted, along with a one-dimensional kaon emission source function. The centrality dependences of the three Gaussian radii are well described by a single linear function of N-part(1/3) with a zero intercept. Imaging analysis shows a deviation from a Gaussian tail at r greater than or similar to 10 fm, although the bulk emission at lower radius is well described by a Gaussian. The presence of a non-Gaussian tail in the kaon source reaffirms that the particle emission region in a heavy-ion collision is extended, and that similar measurements with pions are not solely due to the decay of long-lived resonances.
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