MEASUREMENT OF THE INCLUSIVE CHARGED-CURRENT CROSS-SECTION FOR NEUTRINO AND ANTINEUTRINO SCATTERING ON ISOSCALAR NUCLEONS

被引：46

作者：

AUCHINCLOSS, PS

BLAIR, R

HABER, C

OLTMAN, E

LEUNG, WC

RUIZ, M

MISHRA, SR

QUINTAS, PZ

SCIULLI, FJ

SHAEVITZ, MH

SMITH, WH

MERRITT, FS

OREGLIA, M

REUTENS, P

COLEMAN, R

FISK, HE

LEVINTHAL, D

YOVANOVITCH, DD

MARSH, W

RAPIDIS, PA

WHITE, HB

BODEK, A

BORCHERDING, F

GIOKARIS, N

LANG, K

STOCKDALE, IE

机构：

[1] COLUMBIA UNIV, NEW YORK, NY 10027 USA

[2] UNIV CHICAGO, CHICAGO, IL 60637 USA

[3] FERMI NATL ACCELERATOR LAB, BATAVIA, IL 60510 USA

[4] UNIV ROCHESTER, ROCHESTER, NY 14627 USA

来源：

ZEITSCHRIFT FUR PHYSIK C-PARTICLES AND FIELDS | 1990年 / 48卷 / 03期

关键词：

D O I：

10.1007/BF01572022

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

This paper reports on measurements of the total cross section for the inclusive reaction vμ+N, as a function of incident energy. Neutrinos and antineutrinos with energy in the range 30-300 GeV were produced in the 1982 Fermilab narrow-band neutrino beamline. A total of 35 000 neutrino and 7000 antineutrino interactions were recorded in the CCFR detector located in Lab E. The incident neutrino flux was determined by methods similar to those used in previous experiments. The rate of increase with energy of the total cross section (σ/Ev) in the range 30 to 75 GeV was determined to be 0.659±0.005(stat)±0.039(syst)×10-38 cm2/GeV and 0.307±0.008(stat)±0.020(syst)×10-38 cm2/GeV for incident neutrinos and antineutrinos, respectively. The 5.9% systematic errors are due primarily to uncertainties in the flux intensity measurement. The energy dependence of the cross section in the region Eν=100-300 GeV was found to be linear, as determined by relative normalization techniques. A weighted average of our previous and present measurement for the total ν-N cross section yields: {Mathematical expression}. © 1990 Springer-Verlag.

引用

页码：411 / 431

页数：21

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