Induced radioactive continuum background in the integral spectrometer (SPI) germanium detectors

被引:2
作者
Diallo, N
Jean, P
Legrain, R
Cordier, B
Vedrenne, G
Kandel, B
Salassi-Sennou, S
机构
[1] CEA Saclay, SAp, DAPNIA, DSM, F-91191 Gif Sur Yvette, France
[2] UPS, CNRS, Ctr Etud Spatiale Rayonnements, F-31029 Toulouse, France
[3] CEA Saclay, SPhN, DAPNIA, DSM, F-91191 Gif Sur Yvette, France
[4] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
关键词
Computer simulation - Cosmic ray detectors - Germanium - Monte Carlo methods - Neutron detectors - Protons;
D O I
10.1016/S0168-9002(00)00539-8
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
This paper presents a detailed study of the beta decay continuum background in a spaceborn Ge spectrometer (SPI) and methods for its reduction. In the nuclear gamma -ray line energy range (10 keV, 20 MeV), much of the continuum background in the Ge spectrometers is due to the cosmic-ray generated protons and neutrons interacting in the detectors themselves. We have performed Monte Carlo simulations to calculate the neutron spectrum inside the EGO shield of the spectrometer SPI, thus allowing the calculation of the continuum background induced by the beta (-) and beta (+) decays of the Ge residuals nuclides. It is shown that if we use the Pulse Shape Discrimination (PSD) and energetic signatures in energy ranges well chosen to reduce the background, the main effect is an improvement of the sensitivity of SPI. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:545 / 553
页数:9
相关论文
共 13 条
[1]   HETC - HIGH-ENERGY TRANSPORT CODE [J].
ARMSTRONG, TW ;
CHANDLER, KC .
NUCLEAR SCIENCE AND ENGINEERING, 1972, 49 (01) :110-+
[2]   NUBASE: A database of nuclear and decay properties [J].
Audi, G ;
Bersillon, O ;
Blachot, J ;
Wapstra, AH .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1996, 369 (2-3) :511-515
[3]  
BERSILLON O, 1996, 2 C ACC DRIV TRANS T
[4]  
BRIESMEISTER JF, 1986, LA73967 LANL
[5]  
EVANS RD, 1992, ATOMIC NUCL
[6]  
*GEANT, GEANT316 CERN
[7]  
Jean P., 1996, THESIS U P SABATIER
[8]   The INTEGRAL experiment [J].
Lavigne, JM ;
Jean, P ;
Kandel, B ;
Borrel, V ;
Roques, JP ;
Lichti, G ;
Schonfelder, V ;
Diehl, R ;
Georgii, R ;
Kirchner, T ;
Durouchoux, P ;
Cordier, B ;
Diallo, N ;
Sanchez, F ;
Payne, B ;
Leleux, P ;
Teegarden, B ;
Matteson, J ;
Slassi-Sennou, S ;
Skinner, G ;
Connell, P .
NUCLEAR PHYSICS B, 1998, :69-79
[9]  
LEDERER SM, 1978, TABLE ISOTOPES
[10]   The spectrometer SPI of the INTEGRAL mission [J].
Lichti, GG ;
Schonfelder, V ;
Diehl, R ;
Georgii, R ;
Kirchner, T ;
Vedrenne, G ;
Mandrou, P ;
vonBallmoos, P ;
Jean, P ;
Albernhe, F ;
Durouchoux, P ;
Cordier, B ;
Diallo, N ;
Sanchez, F ;
Leleux, P ;
Caraveo, PA ;
Teegarden, B ;
Matteson, J ;
Lin, R ;
Skinner, GK ;
Connell, P .
GAMMA-RAY AND COSMIC-RAY DETECTORS, TECHNIQUES, AND MISSIONS, 1996, 2806 :217-233