By M. Barone
Court cases of the seventh overseas convention on ICATPP-7, held October 15-19, 2001 in Villa, Olmo, Como, Italy. good points brand new know-how purposes to radiation detection.
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Additional resources for Advanced Technology and Particle Physics
This transfer function F (R, d, ip) is related to the rigidity R of the particle, and to the detecting position. 1 Cosmic Ray Access CR detectors design and performance are different in relation to their location. If the detector is located on the Earth surface his aim to study primary CR flux and composition for example will be persued only with the detection of secondary CR products of the shower occurred in the atmosphere. This will be followed by the reconstruction of the primary vertex obtaining the energy of the particle from the number of secondaries.
This atomic state interferometer n ' 1 2 uses twophoton velocity selective Raman transitions 13 , to manipulate atoms while keeping them in long-lived ground states. 1 Principle of a light pulse matter-wave interferometer Light-pulse interferometers work on the principle that when an atom absorbs or emits a photon momentum must be conserved between the atom and the light field. Consequently, an atom which emits (absorbs) a photon of momentum hkeff will receive a momentum impulse of dp = —hkeff(+hkeff) .
Snadden et al, Phys. Rev. Lett. 8 1 , 971 (1998). M. Sagnac, Compt. Rend. Acad. Sci. 157, 708 (1913). THE GLAST G A M M A RAY LARGE A R E A TELESCOPE S. BREZ, R. N. OMODEI, N. LUMB, L. BALDINI, L. LATRONICO INFN Sez. Pisa Via Livornese 1291 56010 S. Piero a Grado (Pisa) For the Italian GLAST Collaboration The Gamma-ray Large Area Space Telescope (GLAST) is an international space mission that will study the cosmos in the energy range 10 KeV — 300 GeV, the upper end of which is one of the last poorly observed regions of the celestial electromagnetic spectrum to be explored.
Advanced Technology and Particle Physics by M. Barone