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High precision particle astrophysics as a new window on the universe with an Antimatter Large Acceptance Detector In Orbit (ALADInO)
/ Battiston, R (Trento U. ; TIFPA-INFN, Trento) ; Bertucci, B (Perugia U. ; INFN, Perugia) ; Adriani, O (Florence U. ; INFN, Florence) ; Ambrosi, G (INFN, Perugia) ; Baoudoy, B (IRFU, Saclay) ; Blasi, P (GSSI, Aquila) ; Boezio, M (INFN, Trieste) ; Campana, D (INFN, Naples) ; Derome, L (LPSC, Grenoble) ; De Mitri, I (GSSI, Aquila) et al.
Multimessenger astrophysics is based on the detection, with the highest possible accuracy, of the cosmic radiation. During the last 20 years, the advent space-borne magnetic spectrometers in space (AMS-01, Pamela, AMS-02), able to measure the charged cosmic radiation separating matter from antimatter, and to provide accurate measurement of the rarest components of Cosmic Rays (CRs) to the highest possible energies, have become possible, together with the ultra-precise measurement of ordinary CRs. [...]
2021 - 32 p.
- Published in : Exp. Astron.: 51 (2021) , pp. 1299-1330
- Published in : Exp. Astron.: 51 (2021) , pp. 1331-1332
Fulltext: Publication - PDF; Erratum - PDF;
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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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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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The cosmic ray primary composition between $10^{15}$ and $10^{16}$ ev from Extensive Air Showers electromagnetic and TeV muon data
/ 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 cosmic ray primary composition in the energy range between 10/sup 15/ and 10/sup 16/ eV, i.e., around the "knee" of the primary spectrum, has been studied through the combined measurements of the EAS-TOP air shower array (2005 m a.s.l., 10/sup 5/ m/sup 2/ collecting area) and the MACRO underground detector (963 m a.s.l., 3100 m w.e. of minimum rock overburden, 920 m/sup 2/ effective area) at the National Gran Sasso Laboratories. [...]
2004
- Published in : Astropart. Phys. 20 (2004) 641-52
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The $N^{O}E$ Detector for a long baseline neutrino oscillation experiment
/ De Cataldo, G (Bari U. ; INFN, Bari) ; Favuzzi, C (Bari U. ; INFN, Bari) ; Fusco, P (Bari U. ; INFN, Bari) ; Giglietto, N (Bari U. ; INFN, Bari) ; Loparco, F (Bari U. ; INFN, Bari) ; Rainó, A (Bari U. ; INFN, Bari) ; Mazziotta, M N (Bari U. ; INFN, Bari) ; Panunzio, I (Bari U. ; INFN, Bari) ; Spinelli, P (Bari U. ; INFN, Bari) ; Margiotta, A (Bologna U. ; INFN, Bologna) et al.
CERN-SPSC-98-32; LNGS-LOI-99-3-ADD-2; SPSC-M-619.-
Geneva : CERN, 1999 - 11 p.
Fulltext: PDF;
In : 36th INFN Eloisatron Project Workshop : New Detectors "Ettore Majorana", Erice, Italy, 1 - 7 Nov 1997, pp.29-66
- Please contact the library if you need to access this document.
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