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1.
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A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
/ Aalbers, J. (SLAC ; KIPAC, Menlo Park) ; AbdusSalam, S.S. (Shahid Beheshti U.) ; Abe, K. (Kamioka Observ. ; Tokyo U., IPMU) ; Aerne, V. (Zurich U.) ; Agostini, F. (U. Bologna, DIFA ; INFN, Bologna) ; Maouloud, S. Ahmed (Paris U., VI-VII) ; Akerib, D.S. (SLAC ; KIPAC, Menlo Park) ; Akimov, D.Yu. (Moscow Phys. Eng. Inst.) ; Akshat, J. (Purdue U.) ; Musalhi, A.K. Al (Oxford U.) et al.
The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for Weakly Interacting Massive Particles (WIMPs), while featuring extensive sensitivity to many alternative dark matter candidates. [...]
arXiv:2203.02309; INT-PUB-22-003; FERMILAB-PUB-22-112-PPD-QIS-T.-
2022-12-15 - 77 p.
- Published in : J. Phys. G 50 (2023) 013001
Fulltext: 2203.02309 - PDF; jt - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
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2.
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ICARUS 600 ton: A status report
/ Vignoli, C (Pavia U. ; INFN, Pavia) ; Arneodo, F (Gran Sasso) ; Badertscher, A (ETH, Zurich (main)) ; Barbieri, E (U. Pavia (main) ; INFN, Pavia) ; Benetti, P (Pavia U. ; INFN, Pavia) ; Borio di Tigliole, A (Milan Polytechnic) ; Brunetti, R (Pavia U. ; INFN, Pavia) ; Bueno, A (ETH, Zurich (main)) ; Calligarich, E (Pavia U. ; INFN, Pavia) ; Campanelli, Mario (ETH, Zurich (main)) et al.
/ICARUS
The goal of the ICARUS Project is the installation of a multi-kiloton LAr TPC in the underground Gran Sasso Laboratory. The programme foresees the realization of the detector in a modular way. [...]
2000 - 5 p.
- Published in : Nucl. Phys. B, Proc. Suppl. 85 (2000) 119-124
External link: ADSABS
In : 6th Topical Seminar on Neutrino and Astroparticle Physics, San Miniato, Italy, 17 - 21 May 1999, pp.119-124
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3.
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The liquid argon TPC for the ICARUS experiment
/ Arneodo, F (INFN, Aquila ; L'Aquila U.) ; Benetti, P (INFN, Pavia ; Pavia U.) ; Bettini, A (INFN, Padua ; Padua U.) ; Borio, A (INFN, Pavia ; Pavia U.) ; Calligarich, E (INFN, Pavia ; Pavia U.) ; Carpanese, C (INFN, Padua ; Padua U.) ; Casagrande, F (Frascati) ; Cavalli, D (INFN, Milan ; Milan U.) ; Cavanna, F (INFN, Aquila ; L'Aquila U.) ; Cennini, P (CERN) et al.
The ICARUS project aims at the realisation of a large liquid argon TPC to be run at the Underground Laboratories of Gran Sasso in Italy. An intense R&D; activity has put on firm grounds this new detector technology and experimentally confirmed its feasibility on a few ton scale. [...]
1997 - 9 p.
- Published in : Nucl. Phys. B, Proc. Suppl. B 54 (1997) 95-104
In : 6th Topical Seminar on Experimental Apparatus for Particle Physics and Astrophysics, San Miniato, Italy, 20 - 24 May 1996, pp.95-104
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4.
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First Axion Results from the XENON100 Experiment
/ XENON100 Collaboration
We present the first results of searches for axions and axion-like-particles with the XENON100 experiment. The axion-electron coupling constant, $g_{Ae}$, has been tested by exploiting the axio-electric effect in liquid xenon. [...]
arXiv:1404.1455.-
2014-09-09 - 7 p.
- Published in : Phys. Rev. D
Fulltext: PDF; External link: Preprint
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5.
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ICARUS T600 (CNGS2) Status Report
/ CNGS2 Collaboration
Since the last presentation to the SPSC committee, the ICARUS T600 detector assembly has progressed up to its completion. [...]
CERN-SPSC-2009-023 ; SPSC-SR-049.
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2009.
Fulltext
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6.
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7.
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8.
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9.
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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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10.
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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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