By M. Barone
Complaints of the seventh overseas convention on ICATPP-7, held October 15-19, 2001 in Villa, Olmo, Como, Italy. gains brand new know-how functions to radiation detection.
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Table 1. T h e 3 different trigger levels adopted in the GLAST Large Area Telescope. 27 3 Summary of GLAST Science Topics The universe is largely transparent to gamma rays in the energy range of GLAST. Energetic sources near the edge of the visible universe can be detected by the light of their gamma rays. There are good reason to expect that GLAST will see known classes of sources up to redshift 5, or even greater if the sources existed at earlier times. The small interaction cross section for gamma rays can provide a direct view into nature's highest energy accelerators.
4. 5. 6. 7. P. Norris et al, astro-ph/9912136 (1999) A. Moiseev et al, astro-ph/9912138 (1999) A. Moiseev et al, astro-ph/9912139 (1999) J. F. W. W. Stecker et al, astro-ph/9909157 (1999) T. Kamae et al, astro-ph/9901187 (1999) T H E A N T I C O I N C I D E N C E SHIELD OF T H E PAMELA SATELLITE E X P E R I M E N T SCFAB, KTH J. L U N D A N D M. se Sweden The PAMELA experiment consists of a magnetic spectrometer, a transition radiation detector, an electromagnetic imaging calorimeter with a shower-tail catcher and a scintillator-based time-of-flight system.
Schematic of the atomic Sagnac interferometer at Yale 9 on left. Individual signals from the outputs of the two interferometer(gray lines), and difference of the two signals corresponding to a pure rotation signal (black line) versus rotation rate. It should be noted that this phase shift does not depend on the atomic initial velocity or on the mass of the particle. Recently, atomic gravimeter with comparable accuracy than best comer cube has been achieved 10 . The main limitation of this kind of gravimeter on earth is is due to spurious acceleration from the reference platform.
Advanced Technology and Particle Physics by M. Barone