By M. Barone
Court cases of the seventh foreign convention on ICATPP-7, held October 15-19, 2001 in Villa, Olmo, Como, Italy. positive factors modern know-how purposes to radiation detection.
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H Y P E R : ATOM I N T E R F E R O M E T R Y I N SPACE A. LANDRAGIN, A. CLAIRON, N. DIMARCQ, P. TEYSSANDIER, C. M. RASEL, W. J. BORDE, P. TOURRENC Universite Pierre et Marie Curie, Equipe de Relativite, Gravitation et Astrophysique, France P. BOUYER Laboratoire Charles Fabry de I'Institut d'Optique, France M. CALDWELL, R. BINGHAM, B. KENT, M. SANDFORD Rutherford Appleton Laboratory, UK England Bureau International P. WOLF des Poids et Mesures, Sevres, France S. AIREY, G. BAGNASCO ESTEC, ESA, The Netherlands The objective of the HYPER project is to use the very high sensitivity of the atomic interferometry in space for research in fundamental physics This project is sustained by many scientists in the atomic physics community x and by ESA.
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. GLAST will have an imaging gamma-ray telescope vastly more capable than instruments flown previously. The main instrument, the Large Area Telescope (LAT), will have superior area, angular resolution, field of view, and dead time that together will provide a factor of 60 or more advance in sensitivity, and capability for the study of transient phenomena.
SANDFORD Rutherford Appleton Laboratory, UK England Bureau International P. WOLF des Poids et Mesures, Sevres, France S. AIREY, G. BAGNASCO ESTEC, ESA, The Netherlands The objective of the HYPER project is to use the very high sensitivity of the atomic interferometry in space for research in fundamental physics This project is sustained by many scientists in the atomic physics community x and by ESA. After a short introduction, the second part will describe the recent development in atom interferometry.