PRODUCTION OF DSSTAR- MESONS IN ANTINEUTRINO NEON CHARGED CURRENT INTERACTIONS

被引:6
|
作者
ASRATYAN, AE
MARAGE, P
NEVEU, M
AMMOSOV, VV
ANDRYAKOV, AD
BATON, JP
BERGGREN, M
BURTOVOY, VS
COGHEN, T
ERRIQUEZ, O
GAPIENKO, GS
GAPIENKO, VA
GUY, J
JONES, GT
KAFTANOV, VS
KLYUKHIN, VI
KOROTKOV, VA
KRUTCHININ, SP
KUBANTSEV, MA
MAKHLUEVA, IV
MORRISON, DRO
PITUKHIN, PV
SACTON, J
VARVELL, KE
VENUS, W
WALLENBORN, G
WILLOCQ, S
WITTEK, W
ZAETZ, VG
机构
[1] UNIV LIBRE BRUXELLES,VRIJE UNIV BRUSSEL,INTER UNIV INST HIGH ENERGIES,B-1050 BRUSSELS,BELGIUM
[2] CENS,DEPT PHYS PARTICULES ELEMENT,F-91191 GIF SUR YVETTE,FRANCE
[3] SERPUKHOV HIGH ENERGY PHYS INST,SERPUKHOV 142284,USSR
[4] UNIV STOCKHOLM,INST PHYS,S-11346 STOCKHOLM,SWEDEN
[5] INST NUCL PHYS,PL-30055 KRAKOW,POLAND
[6] UNIV BARI,DIPARTMENTO FIS,I-70126 BARI,ITALY
[7] IST NAZL FIS NUCL,BARI,ITALY
[8] RUTHERFORD APPLETON LAB,DIDCOT OX11 0QX,OXON,ENGLAND
[9] UNIV BIRMINGHAM,BIRMINGHAM B15 2TT,W MIDLANDS,ENGLAND
[10] CERN,CH-1211 GENEVA 23,SWITZERLAND
[11] MAX PLANCK INST PHYS & ASTROPHYS,W-8000 MUNICH 40,GERMANY
关键词
D O I
10.1016/0370-2693(91)91931-K
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Evidence of the production of the D(s)*-(2111) meson in nuBAR-mu-Ne collisions is presented. The D(s)*- production rate times the D(s)- --> PHI-pi- branching fraction is estimated to be (2.3 +/- 0.7) x 10(-3) of all charged currents having a hadronic mass W above 3 GeV.
引用
收藏
页码:525 / 530
页数:6
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