K(0) PRODUCTION IN ONE-PRONG TAU-DECAYS

被引:19
|
作者
BUSKULIC, D
CASPER, D
DEBONIS, I
DECAMP, D
GHEZ, P
GOY, C
LEES, JP
MINARD, MN
ODIER, P
PIETRZYK, B
ARIZTIZABAL, F
CHMEISSANI, M
CRESPO, JM
EFTHYMIOPOULOS, I
FERNANDEZ, E
FERNANDEZBOSMAN, M
GAITAN, V
GARRIDO, L
MARTINEZ, M
MATTISON, T
ORTEU, S
PACHECO, A
PADILLA, C
PASCUAL, A
TEUBERT, F
CREANZA, D
DEPALMA, M
FARILLA, A
IASELLI, G
MAGGI, G
MARINELLI, N
NATALI, S
NUZZO, S
RANIERI, A
RASO, G
ROMANO, F
RUGGIERI, F
SELVAGGI, G
SILVESTRIS, L
TEMPESTA, P
ZITO, G
CHAI, Y
HUANG, D
HUANG, X
LIN, J
WANG, T
XIE, Y
XU, D
XU, R
ZHANG, J
机构
[1] UNIV AUTONOMA BARCELONA, INST FIS ALTES ENERGIES, E-08193 BARCELONA, SPAIN
[2] INFN, DIPARTIMENTO FIS, I-70126 BARI, ITALY
[3] CERN, EUROPEAN LAB PARTICLE PHYS, CH-1211 GENEVA 23, SWITZERLAND
[4] UNIV CLERMONT FERRAND, PHYS CORPUSCULAIRE LAB, CNRS, IN2P3, F-63177 CLERMONT FERRAND, FRANCE
[5] NIELS BOHR INST, DK-2100 COPENHAGEN, DENMARK
[6] ECOLE POLYTECH, PHYS NUCL & HAUTES ENERGIES LAB, CNRS, IN2P3, F-91128 PALAISEAU, FRANCE
[7] CHINESE ACAD SCI, INST HIGH ENERGY PHYS, BEIJING, PEOPLES R CHINA
[8] DEMOKRITOS NATL CTR SCI RES, ATHENS, GREECE
[9] UNIV WASHINGTON, SEATTLE, WA 98195 USA
[10] UNIV TURIN, IST FIS GEN, I-10124 TURIN, ITALY
[11] CNR, IST COSMOGEOFIS, TURIN, ITALY
[12] KANGNUNG NATL UNIV, KANGNUNG, SOUTH KOREA
[13] CERN, DIV PPE, CH-1211 GENEVA 23, SWITZERLAND
[14] UNIV EDINBURGH, DEPT PHYS, EDINBURGH EH8 9JZ, MIDLOTHIAN, SCOTLAND
[15] UNIV FLORENCE, INFN, DIPARTIMENTO FIS, I-50125 FLORENCE, ITALY
[16] FLORIDA STATE UNIV, SUPERCOMP COMPUTAT RES INST, TALLAHASSEE, FL 32306 USA
[17] INFN, LAB NAZL, I-00044 FRASCATI, ITALY
[18] UNIV HEIDELBERG, INST HOCHENERGIEPHYS, D-69120 HEIDELBERG, GERMANY
[19] UNIV MAINZ, INST PHYS, D-55099 MAINZ, GERMANY
[20] FAC SCI LUMINY, CTR PHYS PARTICULES, CNRS, IN2P3, F-13288 MARSEILLE, FRANCE
[21] WERNER HEISENBERG INST, MAX PLANCK INST PHYS, D-80805 MUNICH, GERMANY
[22] SCUOLA NORMALE SUPER PISA, I-56010 PISA, ITALY
[23] UNIV LONDON ROYAL HOLLOWAY & BEDFORD NEW COLL, DEPT PHYS, EGHAM TW20 0EX, SURREY, ENGLAND
[24] UNIV SIEGEN, FACHBEREICH PHYS, D-57068 SIEGEN, GERMANY
[25] INFN, I-34127 TRIESTE, ITALY
[26] UNIV GLASGOW, DEPT PHYS & ASTRON, GLASGOW G12 8QQ, SCOTLAND
[27] UNIV LONDON IMPERIAL COLL SCI TECHNOL & MED, DEPT PHYS, LONDON SW7 2BZ, ENGLAND
[28] UNIV INNSBRUCK, INST EXPTL PHYS, A-6020 INNSBRUCK, AUSTRIA
[29] UNIV LANCASTER, DEPT PHYS, LANCASTER LA1 4YB, ENGLAND
[30] UNIV PARIS 11, ACCELERATEUR LINEAIRE LAB, CNRS, IN2P3, F-91405 ORSAY, FRANCE
[31] UNIV PISA, INFN, DIPARTIMENTO FIS, I-56010 PISA, ITALY
[32] CTR ETUD SACLAY, DAPNIA, SERV PHYS PARTICULES, F-91191 GIF SUR YVETTE, FRANCE
[33] RUTHERFORD APPLETON LAB, DEPT PARTICLE PHYS, DIDCOT OX11 0QX, OXON, ENGLAND
[34] UNIV CALIF SANTA CRUZ, INST PARTICLE PHYS, SANTA CRUZ, CA 95064 USA
[35] UNIV SHEFFIELD, DEPT PHYS, SHEFFIELD S3 7RH, S YORKSHIRE, ENGLAND
[36] UNIV WISCONSIN, DEPT PHYS, MADISON, WI 53706 USA
[37] UNIV TRIESTE, DIPARTIMENTO FIS, I-34127 TRIESTE, ITALY
基金
中国国家自然科学基金;
关键词
D O I
10.1016/0370-2693(94)90882-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
From a sample of about 75000 tau decays identified with the ALEPH detector, K0 production in 1-prong hadronic decays is investigated by tagging the K(L)0 component in a hadronic calorimeter. Results are given for the final states nu(tau)h-K0 and nu(tau)h-pi0K0 where the h- is separated into pi and K contributions by means of the dE/dx measurement in the central detector. The resulting branching ratios are: (B(tau) --> nu(tau)pi-K0) = (0.88 +/- 0.14 +/- 0.09)%, (B(tau) --> nu(tau)K-K0) = (0.29 +/- 0.12 +/- 0.03)%, (Btau --> nu(tau)pi-pi0K0) = (0.33 +/- 0.14 +/- 0.07)% and (B(tau) --> nu(tau)K-pi0K0) = (0.05 +/- 0.05 +/- 0.01)%. The K* decay rate in the K0pi channel agrees with that in the Kpi0 mode: the combined value for the branching ratio is (Btau --> nu(tau)K*-) = (1.45 +/- 0.13 +/- 0.11)%.
引用
收藏
页码:219 / 227
页数:9
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