STUDY OF D-ASTERISK(2010)(+/-)-PRODUCTION IN EP-COLLISIONS AT HERA

被引:50
作者
DERRICK, M
KRAKAUER, D
MAGILL, S
MIKUNAS, D
MUSGRAVE, B
REPOND, J
STANEK, R
TALAGA, RL
ZHANG, H
AYAD, R
BARI, G
BASILE, M
BELLAGAMBA, L
BOSCHERINI, D
BRUNI, A
BRUNI, G
BRUNI, P
ROMEO, GC
CASTELLINI, G
CHIARINI, M
CIFARELLI, L
CINDOLO, F
CONTIN, A
CORRADI, M
GIALAS, I
GIUSTI, P
IACOBUCCI, G
LAURENTI, G
LEVI, G
MARGOTTI, A
MASSAM, T
NANIA, R
NEMOZ, C
PALMONARI, F
POLINI, A
SARTORELLI, G
TIMELLINI, R
GARCIA, YZ
ZICHICHI, A
BARGENDE, A
CRITTENDEN, J
DESCH, K
DIEKMANN, B
DOEKER, T
ECKERT, M
FELD, L
FREY, A
GEERTS, M
GEITZ, G
GROTHE, M
机构
[1] UNIV BOLOGNA, BOLOGNA, ITALY
[2] IST NAZL FIS NUCL, I-40126 BOLOGNA, ITALY
[3] UNIV BONN, INST PHYS, W-5300 BONN, GERMANY
[4] UNIV BRISTOL, HH WILLS PHYS LAB, BRISTOL BS8 1TL, AVON, ENGLAND
[5] BROOKHAVEN NATL LAB, UPTON, NY 11973 USA
[6] IST NAZL FIS NUCL, COSENZA, ITALY
[7] UNIV CALABRIA, I-87036 COSENZA, ITALY
[8] COLUMBIA UNIV, NEVI LABS, IRVINGTON, NY USA
[9] INST NUCL PHYS, KRAKOW, POLAND
[10] AGH UNIV SCI & TECHNOL, FAC PHYS & NUCL TECH, KRAKOW, POLAND
[11] JAGIELLONIAN UNIV, DEPT PHYS, KRAKOW, POLAND
[12] DESY, W-2000 HAMBURG, GERMANY
[13] DESY, INST HOCHENERGIEPHYS, O-1615 ZEUTHEN, GERMANY
[14] UNIV FLORENCE, FLORENCE, ITALY
[15] IST NAZL FIS NUCL, I-50125 FLORENCE, ITALY
[16] IST NAZL FIS NUCL, LAB NAZL FRASCATI, I-00044 FRASCATI, ITALY
[17] UNIV FREIBURG, FAK PHYS, W-7800 FREIBURG, GERMANY
[18] UNIV GLASGOW, DEPT PHYS & ASTRON, GLASGOW, LANARK, SCOTLAND
[19] UNIV HAMBURG, INST EXPTL PHYS 1, HAMBURG, GERMANY
[20] UNIV HAMBURG, INST EXPTL PHYS 2, W-2000 HAMBURG, GERMANY
[21] UNIV LONDON IMPERIAL COLL SCI & TECHNOL, HIGH ENERGY NUCL PHYS GRP, LONDON, ENGLAND
[22] UNIV IOWA, DEPT PHYS & ASTRON, IOWA CITY, IA 52242 USA
[23] FORSCHUNGSZENTRUM JULICH, FORSCHUNGSZENTRUM, INST KERNPHYS, W-5170 JULICH, GERMANY
[24] KOREA UNIV, SEOUL 136701, SOUTH KOREA
[25] LOUISIANA STATE UNIV, DEPT PHYS & ASTRON, BATON ROUGE, LA 70803 USA
[26] UNIV AUTONOMA MADRID, DEPT FIS TEOR, MADRID, SPAIN
[27] UNIV MANITOBA, DEPT PHYS, WINNIPEG, MB R3T 2N2, CANADA
[28] MCGILL UNIV, DEPT PHYS, MONTREAL, PQ, CANADA
[29] MOSCOW ENGN PHYS INST, MOSCOW 115409, RUSSIA
[30] NIKHEF, AMSTERDAM, NETHERLANDS
[31] UNIV AMSTERDAM, AMSTERDAM, NETHERLANDS
[32] OHIO STATE UNIV, DEPT PHYS, COLUMBUS, OH 43210 USA
[33] UNIV OXFORD, DEPT PHYS, OXFORD, ENGLAND
[34] UNIV PADUA, DIPARTIMENTO FIS, PADUA, ITALY
[35] IST NAZL FIS NUCL, PADUA, ITALY
[36] PENN STATE UNIV, DEPT PHYS, UNIVERSITY PK, PA 16802 USA
[37] UNIV ROMA LA SAPIENZA, DIPARTIMENTO FIS, I-00185 ROME, ITALY
[38] IST NAZL FIS NUCL, I-00185 ROME, ITALY
[39] RUTHERFORD APPLETON LAB, DIDCOT OX11 0QX, OXON, ENGLAND
[40] UNIV CALIF SANTA CRUZ, SANTA CRUZ, CA 95064 USA
[41] UNIV GESAMTHSCH SIEGEN, FACHBEREICH PHYS, W-5900 SIEGEN, GERMANY
[42] TEL AVIV UNIV, SCH PHYS, IL-69978 TEL AVIV, ISRAEL
[43] UNIV TOKYO, INST NUCL STUDY, TOKYO, JAPAN
[44] TOKYO METROPOLITAN UNIV, DEPT PHYS, TOKYO, JAPAN
[45] UNIV TURIN, DIPARTIMENTO FIS SPERIMENTALE, TURIN, ITALY
[46] IST NAZL FIS NUCL, I-10125 TURIN, ITALY
[47] UNIV TURIN, FAC SCI 2, ALESSANDRIA, ITALY
[48] IST NAZL FIS NUCL, ALESSANDRIA, ITALY
[49] UNIV TORONTO, DEPT PHYS, TORONTO, ON, CANADA
[50] UCL, DEPT PHYS & ASTRON, LONDON, ENGLAND
基金
美国国家科学基金会;
关键词
D O I
10.1016/0370-2693(95)00253-H
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the first observation of charmed mesons with the ZEUS detector at HERA using the decay channel D*(+) --> (D-0 --> K(-)pi(+)) pi(+) (+ c.c.). Clear signals in the mass difference Delta M=M(D*)-M(D-0) as well as in the M(K pi) distribution at the D-0 mass are found. The ep cross section for inclusive D*(+/-) production with Q(2) < 4 GeV2 in the gamma p centre-of-mass energy range 115 < W < 275 GeV has been determined to be (32+/-7(-7)(+4)) nb in the kinematic region {pr(D*) greater than or equal to 1.7 GeV, \pi(D*)\ < 1.5}. Extrapolating outside this region, assuming a mass of the charm quark of 1.5 GeV, we estimate the ep charm cross section to be sigma(ep --> c $($) over bar$$ cX)=(0.45+/-0.11(-0.22)(+0.37)) mu b at root s=296 GeV and [W]=198 GeV. The average gamma p charm cross section sigma(gamma p --> c $($) over bar$$ cX) is found to be (6.3+/-2.2(-3.0)(+6.3)) mu b at [W]=163 GeV and (16.9+/-5.2(-8.5)(+13.9)) mu b at [W]=243 GeV. The increase of the total charm photoproduction cross section by one order of magnitude with respect to low energy data experiments is well described by QCD NLO calculations using singular gluon distributions in the proton.
引用
收藏
页码:225 / 237
页数:13
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