ENERGY AND FLUENCE DETERMINATION OF FAST-NEUTRONS FROM 44 GEV C-12 + CU INTERACTIONS BY CR-39 DETECTOR STACK

被引：0

作者：

GUO, SL

HAO, XH

WANG, YL

SHEN, GR

BARTH, H

BAUMBACH, H

BRANDT, R

BUTSEV, VS

HAASE, G

HECK, M

KRIVOPUSTOV, MI

KULAKOV, BA

LANGROCK, EJ

PILLE, F

机构：

[1] TH LEIPZIG,SEKT NAT WISSENSCH,LEIPZIG,GERMANY

[2] UNIV MARBURG,W-3550 MARBURG,GERMANY

[3] DUBNA JOINT NUCL RES INST,DUBNA,USSR

来源：

NUCLEAR TRACKS AND RADIATION MEASUREMENTS | 1991年 / 19卷 / 1-4期

关键词：

FAST NEUTRONS; 44 GEV 12C + CU; 400 KEV D + T; CR-39; DETECTOR;

D O I：

暂无

中图分类号：

TL [原子能技术]; O571 [原子核物理学];

学科分类号：

0827 ; 082701 ;

摘要：

Copious amounts of fast neutrons are produced in relativistic heavy ion interactions, which bring about information on the mechanisms of relativistic heavy ion interactions and could constitute considerable radiation hazard. In order to determine their energy and yield, we have detected with a CR-39 detector stack neutrons produced in 44 GeV C-12 + Cu interactions at the SYNCHROPHASOTRON, Joint Institute for Nuclear Research (JINR), Dubna, USSR and the neutrons from 400 keV d + T reactions at the Cockroft-Walton, China Institute of Atomic Energy, Beijing, China, for comparison.

引用

页码：615 / 618

页数：4