MAX:: Development of a Laue diffraction lens for nuclear astrophysics

被引:5
作者
Barriere, N.
von Ballmoos, P.
Skinner, G.
Smither, B.
Bastie, P.
Hinglais, E.
Abrosimov, N.
Alvarez, J. M.
Andersen, K.
Courtois, P.
Halloin, H.
Harris, M.
Isern, J.
Jean, P.
Knoedlseder, J.
Ubertini, P.
Vedrenne, G.
Weldenspointner, G.
Wunderer, C.
机构
[1] Univ Toulouse 3, Ctr Etud Spatiale Rayonnements, F-31028 Toulouse 4, France
[2] Argonne Natl Lab, Argonne, IL 60439 USA
[3] Univ Grenoble 1, Spectrometrie Phys Lab, F-38402 St Martin Dheres, France
[4] Ctr Natl Etud Spatiales, F-31401 Toulouse, France
[5] Inst Kristallzuchtung, D-12489 Berlin, Germany
[6] Inst Estudis Espacials Catalunya, Barcelona 8034, Spain
[7] Inst Max Von Laue Paul Langevin, F-38042 Grenoble, France
[8] Coll France, Federat Rech APC, F-75231 Paris, France
[9] Ist Astrofis Spaziale & Fis Cosm, I-00133 Rome, Italy
[10] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
关键词
instrumentation; gamma-ray lane lens; gamma-ray astrophysics; mosaic crystals;
D O I
10.1016/j.nima.2006.05.150
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The next generation of instrumentation for nuclear astrophysics will have to achieve an improvement in sensitivity by a factor of 10-100 over present technologies. With the focusing gamma-ray telescope MAX we take up this challenge and propose to combine the required sensitivity with high spectral and angular resolution, and the capability to measure the polarization of the photons. MAX is a space-borne crystal diffraction telescope, featuring a broad-band Lane lens optimized for the observation of compact sources in two wide energy bands of high astrophysical relevance. Gamma rays will be focused from the large collecting area of a crystal diffraction lens onto a very small detector volume. As a consequence, the signal to background ratio is greatly enhanced, leading to unprecedented sensitivities. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码:333 / 336
页数:4
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