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MASS-SAT: Matter-antimatter space spectrometer on satellite
/ Basini, G (Frascati) ; Candusso, M (Frascati) ; Massimo Brancaccio, F (Frascati) ; Ricci, M (Frascati) ; Bocciolini, M (Florence U. ; INFN, Florence) ; Spillantini, P (Florence U. ; INFN, Florence) ; Wang, Y F (Florence U. ; INFN, Florence) ; Bongiorno, F (Rome U.) ; de Pascale, M P (Rome U., Tor Vergata ; INFN, Rome2) ; Morselli, A (Rome U., Tor Vergata ; INFN, Rome2) et al.
The MASS-SAT Experiment (Matter-Antimatter Space Spectrometer on SATellite) presented here is conceived to search for an experimental answer to many open problems related to both Astrophysics and Physics, through the detection of positrons, antiprotons, nuclei and, overall, antinuclei if they exist. Among these problems there are the hypothesized presence of antigalaxies in the Universe (the matter-antimatter symmetry problem), the existence of black holes as possible antiproton sources (the Hawking effect), the existence of photinos as antiproton sources (related to the dark-matter problem), the understanding of the mechanism of cosmic-ray acceleration in the interstellar medium, the determination of the relative abundancies of isotopes in cosmic rays and many others. [...]
1990-07 - 17 p.
- Published in : Nuovo Cimento B 105 (1990) 779-795
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3.
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Inelastic Diffractive Scattering at Energies of 140 to 175 GeV*
/ Ayres, D S (Argonne National Laboratory, Ilinois) ; Diebold, R (Argonne National Laboratory, Ilinois) ; Cutts, D (Brown University, Rhode Island) ; Lanou, R E (Brown University, Rhode Island) ; Levinson, L J (Brown University, Rhode Island) ; Massimo, J T (Brown University, Rhode Island) ; Litt, J (CERN) ; Meunier, R (CERN) ; Gittelman, B (Cornell University, New York) ; Sogard, M (Cornell University, New York) et al.
1976
- Published in : Phys. Rev. Lett. 37 (1976) 1724
APS Published version, local copy: PDF;
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4.
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PAMELA - A Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics
/ Picozza, P. (Rome U., Tor Vergata) ; Galper, A.M. (Moscow Phys. Eng. Inst.) ; Castellini, G. (IFAC, Florence) ; Adriani, O. (INFN, Florence) ; Altamura, F. (Rome U., Tor Vergata) ; Ambriola, M. (INFN, Bari) ; Barbarino, G.C. (INFN, Naples) ; Basili, A. (Rome U., Tor Vergata) ; Bazilevskaja, G.A. (Lebedev Inst.) ; Bencardino, R. (Rome U., Tor Vergata) et al.
The PAMELA experiment is a satellite-borne apparatus designed to study charged particles in the cosmic radiation with a particular focus on antiparticles. PAMELA is mounted on the Resurs DK1 satellite that was launched from the Baikonur cosmodrome on June 15th 2006. [...]
astro-ph/0608697.-
2006 - 20 p.
- Published in : Astropart. Phys. 27 (2007) 296-315
Access to fulltext document: PDF; External link: astro-ph/0608697 PDF
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5.
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Experimental study of low-pt hadron fragmentation
/ Cutts, D (Brown Univ., Rhode Island, USA) ; Dulude, R S (Brown Univ., Rhode Island, USA) ; Lanou, R E (Brown Univ., Rhode Island, USA) ; Massimo, J T (Brown Univ., Rhode Island, USA) ; Meunier, R (CERN) ; Brenner, A E (Fermi National Accelerator Laboratory, Illinois, USA) ; Carey, D C (Fermi National Accelerator Laboratory, Illinois, USA) ; Elias, J E (Fermi National Accelerator Laboratory, Illinois, USA) ; Garbincius, P H (Fermi National Accelerator Laboratory, Illinois, USA) ; Mikenberg, G (Fermi National Accelerator Laboratory, Illinois, USA) et al.
Geneva : CERN, 1979
- Published in : Phys. Rev. Lett. 49 (1979) 319-322
APS Published version, local copy: PDF;
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6.
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Inclusive double-charge-exchange π- production at 100 GeV/c
/ Cutts, D (Brown Univ. Rhode Island, USA) ; Dulude, R (Brown Univ. Rhode Island, USA) ; Lanou, R E (Brown Univ. Rhode Island, USA) ; Massimo, J T (Brown Univ. Rhode Island, USA) ; Meunier, R (CERN) ; Brenner, A E (Fermi National Accelerator Laboratory, Illinois, USA) ; Carey, D C (Fermi National Accelerator Laboratory, Illinois, USA) ; Elias, J E (Fermi National Accelerator Laboratory, Illinois, USA) ; Garbincius, P H (Fermi National Accelerator Laboratory, Illinois, USA) ; Mikenberg, G (Fermi National Accelerator Laboratory, Illinois, USA) et al.
Geneva : CERN, 1978
- Published in : Phys. Rev. Lett. 40 (1978) 141-144
APS Published version, local copy: PDF;
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7.
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Impact-parameter analysis of elastic scattering from 50 to 175 GeV/c
/ Ayres, D S (Argonne National Laboratory) ; Nelson, B (MIT) ; Gottschalk, B (Northeatern Univ.) ; Anderson, R L (Stanford Linear Accelerator Center) ; Ritson, D M (Stanford Linear Accelerator Center) ; Weitsch, G A (Stanford Linear Accelerator Center) ; Rich, K (Stanford Linear Accelerator Center) ; Gustavson, D (Stanford Linear Accelerator Center) ; Verdier, R (MIT) ; Rosenson, L (MIT) et al.
1976
- Published in : Phys. Rev. D 14 (1976) 3092
APS Published version, local copy: PDF;
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8.
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The cosmic ray proton, helium and CNO fluxes in the 100 TeV energy region from TeV muons and EAS atmospheric Cherenkov light observations of MACRO and EAS-TOP
/ Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the National Gran Sasso Laboratories by means of EAS-TOP (Campo Imperatore, 2005 m a.s.l.) and MACRO (deep underground, 3100 m w.e., the surface energy threshold for a muon reaching the detector being E/sub mu //sup th/ approximately=1.3 TeV). The measurement is based on: (a) the selection of primaries based on their energy/nucleon (i.e., with energy/nucleon sufficient to produce a muon with energy larger than 1.3 TeV) and the reconstruction of the shower geometry by means of the muons recorded by MACRO in the deep underground laboratories; (b) the detection of the associated atmospheric Cherenkov light (C.l.) signals by means of the C.l. [...]
2004
- Published in : Astropart. Phys. 21 (2004) 223-40
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