Fundamental Physics and applications

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Presentation transcript:

Fundamental Physics and applications S. Dell’Agnello, A. Mastroberardino, M. Schioppa, G. Susinno

Fundamental Physics Experiments The smaller the object to investigate the larger the apparatus to use: accelerators + detectors Crystallography Sub-Nuclear Physics source beam beam target target detector detector nλ = 2dsinθ

Particle Physics Experiments To take this kind of picture we need particle detectors with the following characteristics Radiation hard High spatial resolution Sensitivity to charge and neutral particles High time resolution Low cost

Detectors Trigger Tracking Position (resolution better than 100um) Energy Momentum Time of flight (resolution better than 1ns) Trigger Selection of the interesting events Tracking Pattern recognition and reconstruction of the particle track

Metrologia del posizionamento per esperimenti di fisica e satelliti, con enfasi su tecnologie laser Simone Dell’Agnello Coordinator of Technological and Interdisciplinary Research Commissione Scientifica Nazionale 5 (CSN5) INFN-LNF/Cosenza Italian National Institute for Nuclear Physics, Laboratori Nazionali di Frascati (INFN-LNF) Via Enrico Fermi 40, Frascati (Rome), 00044, Italy

SLR/LLR examples S L R LAGEOS (h ~ 6000 km): ToF ~ 0.05 sec Apollo LRA Lunar Laser Ranging: ToF ~ 2.5 sec

APOLLO 11, 14, 15 Apollo 11: 100 CCRs LAGEOS I (‘76; NASA), LAGEOS II (‘92; NASA/ASI) COPERNICUS RETROREFLECTOR ARRAY (for Earth Observation) Flight payload for GPS-2 @INFN-LNF: 32 CCRs (property of Univ. Maryland)

Locations of 1st Gen. Lunar Retroreflector Arrays Lunar Laser Ranging: accurate at ~ 10-11 of Earth-Moon distance Relative sizes and separation of the Earth–Moon. An LLR pulse takes 1.255 sec for the mean orbital distance. Locations of 1st Gen. Lunar Retroreflector Arrays