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Inclusive K(S)(0)K(S)(0) resonance production in ep collisions at HERA

Authors :
Chekanov, S
Derrick, M
Magill, S
Musgrave, B
Nicholass, D
Repond, J
Yoshida, R
Mattingly, MCK
Antonioli, P
Bari, G
Bellagamba, L
Boscherini, D
Bruni, A
Bruni, G
Cindolo, F
Corradi, M
Iacobucci, G
Margotti, A
Nania, R
Polini, A
Antonelli, S
Basile, M
Bindi, M
Cifarelli, L
Contin, A
De Pasquale, S
Sartorelli, G
Zichichi, A
Bartsch, D
Brock, I
Hartmann, H
Hilger, E
Jakob, H-P
Juengst, M
Nuncio-Quiroz, AE
Paul, E
Samson, U
Schoenberg, V
Shehzadi, R
Wlasenko, M
Brook, NH
Heath, GP
Morris, JD
Capua, M
Fazio, S
Mastroberardino, A
Schioppa, M
Susinno, G
Tassi, E
Kim, JY
Ibrahim, ZA
Kamaluddin, B
Abdullah, WATW
Ning, Y
Ren, Z
Sciulli, F
Chwastowski, J
Eskreys, A
Figiel, J
Galas, A
Gil, M
Olkiewicz, K
Stopa, P
Zawiejski, L
Adamczyk, L
Bold, T
Grabowska-Bold, I
Kisielewska, D
Lukasik, J
Przybycien, M
Suszycki, L
Kotanski, A
Slominski, W
Behrens, U
Blohm, C
Bonato, A
Borras, K
Ciesielski, R
Coppola, N
Fang, S
Fourletova, J
Geiser, A
Goettlicher, P
Grebenyuk, J
Gregor, I
Haas, T
Hain, W
Huettmann, A
Januschek, F
Kahle, B
Katkov, II
Klein, U
Koetz, U
Kowalski, H
Lobodzinska, E
Loehr, B
Mankel, R
Melzer-Pellmann, I-A
Miglioranzi, S
Montanari, A
Namsoo, T
Notz, D
Parenti, A
Rinaldi, L
Roloff, P
Rubinsky, I
Santamarta, R
Schneekloth, U
Spiridonov, A
Szuba, D
Szuba, J
Theedt, T
Wolf, G
Wrona, K
Molina, AGY
Youngman, C
Zeuner, W
Drugakov, V
Lohmann, W
Schlenstedt, S
Barbagli, G
Gallo, E
Pelfer, PG
Bamberger, A
Dobur, D
Karstens, F
Vlasov, NN
Bussey, PJ
Doyle, AT
Dunne, W
Forrest, M
Rosin, M
Saxon, DH
Skillicorn, IO
Gialas, I
Papageorgiu, K
Holm, U
Klanner, R
Lohrmann, E
Schleper, P
Schoerner-Sadenius, T
Sztuk, J
Stadie, H
Turcato, M
Foudas, C
Fry, C
Long, KR
Tapper, AD
Matsumoto, T
Nagano, K
Tokushuku, K
Yamada, S
Yamazaki, Y
Barakbaev, AN
Boos, EG
Pokrovskiy, NS
Zhautykov, BO
Aushev, V
Borodin, M
Kadenko, I
Kozulia, A
Libov, V
Lisovyi, M
Lontkovskyi, D
Makarenko, I
Sorokin, I
Verbytskyi, A
Volynets, O
Son, D
de Favereau, J
Piotrzkowski, K
Barreiro, F
Glasman, C
Jimenez, M
Labarga, L
del Peso, J
Ron, E
Soares, M
Terron, J
Zambrana, M
Corriveau, F
Liu, C
Schwartz, J
Walsh, R
Zhou, C
Tsurugai, T
Antonov, A
Dolgoshein, BA
Gladkov, D
Sosnovtsev, V
Stifutkin, A
Suchkov, S
Dementiev, RK
Ermolov, PF
Gladilin, LK
Golubkov, YA
Khein, LA
Korzhavina, IA
Kuzmin, VA
Levchenko, BB
Lukina, OY
Proskuryakov, AS
Shcheglova, LM
Zotkin, DS
Abt, I
Caldwell, A
Kollar, D
Reisert, B
Schmidke, WB
Grigorescu, G
Keramidas, A
Koffeman, E
Kooijman, P
Pellegrino, A
Tiecke, H
Vazquez, M
Wiggers, L
Bruemmer, N
Bylsma, B
Durkin, LS
Lee, A
Ling, TY
Allfrey, PD
Bell, MA
Cooper-Sarkar, AM
Devenish, RCE
Ferrando, J
Foster, B
Korcsak-Gorzo, K
Oliver, K
Robertson, A
Uribe-Estrada, C
Walczak, R
Bertolin, A
Dal Corso, F
Dusini, S
Longhin, A
Stanco, L
Bellan, P
Brugnera, R
Carlin, R
Garfagnini, A
Limentani, S
Oh, BY
Raval, A
Ukleja, J
Whitmore, JJ
Iga, Y
D'Agostini, G
Marini, G
Nigro, A
Cole, JE
Hart, JC
Abramowicz, H
Ingbir, R
Kananov, S
Levy, A
Stern, A
Kuze, M
Maeda, J
Hori, R
Kagawa, S
Okazaki, N
Shimizu, S
Tawara, T
Hamatsu, R
Kaji, H
Kitamura, S
Ota, O
Ri, YD
Costa, M
Ferrero, MI
Monaco, V
Sacchi, R
Solano, A
Arneodo, M
Ruspa, M
Fourletov, S
Martin, JF
Stewart, TP
Boutle, SK
Butterworth, JM
Gwenlan, C
Jones, TW
Loizides, JH
Wing, M
Brzozowska, B
Ciborowski, J
Grzelak, G
Kulinski, P
Luzniak, P
Malka, J
Nowak, RJ
Pawlak, JM
Tymieniecka, T
Ukleja, A
Zarnecki, AF
Adamus, M
Plucinski, P
Eisenberg, Y
Hochman, D
Karshon, U
Brownson, E
Danielson, T
Everett, A
Kcira, D
Reeder, DD
Ryan, P
Savin, AA
Smith, WH
Wolfe, H
Bhadra, S
Catterall, CD
Cui, Y
Hartner, G
Menary, S
Noor, U
Standage, J
Whyte, J
Collaboration, ZEUS
Source :
ResearcherID
Publication Year :
2008

Abstract

Inclusive K_{S};{0}K_{S};{0} production in ep collisions at the DESY ep collider HERA was studied with the ZEUS detector using an integrated luminosity of 0.5 fb;{-1}. Enhancements in the mass spectrum were observed and are attributed to the production of f_{2}(1270)/a_{2};{0}(1320), f_{2};{'}(1525) and f_{0}(1710). Masses and widths were obtained using a fit which takes into account theoretical predictions based on SU(3) symmetry arguments, and are consistent with the Particle Data Group values. The f_{0}(1710) state, which has a mass consistent with a glueball candidate, was observed with a statistical significance of 5 standard deviations. However, if this state is the same as that seen in gammagamma-->K_{S};{0}K_{S};{0}, it is unlikely to be a pure glueball state.

Details

ISSN :
10797114 and 00319007
Volume :
101
Issue :
11
Database :
OpenAIRE
Journal :
PHYSICAL REVIEW LETTERS
Accession number :
edsair.pmid.dedup....24f9dce6ae88981be7b602dec567efc8