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CERN Document Server Sök i 20 journaler efter:  1 - 10nästa  gå till journal: Sökningen tog 0.64 sekunder. 
1.
The magnetized steel and scintillator calorimeters of the MINOS experiment / MINOS Collaboration
The Main Injector Neutrino Oscillation Search (MINOS) experiment uses an accelerator-produced neutrino beam to perform precision measurements of the neutrino oscillation parameters in the 'atmospheric neutrino' sector associated with muon neutrino disappearance. This long-baseline experiment measures neutrino interactions in Fermilab's NuMI neutrino beam with a near detector at Fermilab and again 735 km downstream with a far detector in the Soudan Underground Laboratory in northern Minnesota. [...]
arXiv:0805.3170; FERMILAB-PUB-08-126; FERMILAB-PUB-08-126.- 2008 - 87 p. - Published in : Nucl. Instrum. Methods Phys. Res., A 596 (2008) 190-228 Preprint: PDF;
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2.
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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3.
Calibrations of CR39 and Makrofol nuclear track detectors and search for exotic particles / MACRO Collaboration
We present the final results of the search for exotic massive particles in the cosmic radiation performed with the MACRO underground experiment. Magnetic monopoles and nuclearites flux upper limits obtained with the CR39 nuclear track subdetector, the scintillation and streamer tube subdetectors are given. [...]
2003 - Published in : Nucl. Phys. B, Proc. Suppl. 125 (2003) 217-21
In : 8th Topical Seminar on Innovative Particle and Radiation Detectors, Sienna, Italy, 21 - 24 Oct 2002, pp.217-21 (vol. 125)
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4.
Search for GUT magnetic monopoles and nuclearites with the MACRO experiment / MACRO Collaboration
We present the final results obtained by the MACRO experiment in the search for GUT magnetic monopoles and nuclearites. Several searches were performed with different subdetectors, i.e. [...]
2003 - Published in : Radiat. Meas. 36 (2003) 301-5
In : 21st International Conference on Nuclear Tracks in Solids, New Delhi, India, 21 - 25 Oct 2002, pp.301-5 (vol. 36)
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5.
Search for stellar gravitational collapses with the MACRO detector / MACRO Collaboration
We present the final results of the search for stellar gravitational collapses obtained by the MACRO experiment. The detector was active for a stellar collapse search for more than 11 years and it was sensitive to collapses occurring all over in our galaxy for 8.6 years. [...]
2004 - Published in : Eur. Phys. J. C 37 (2004) 265-72
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6.
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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7.
A combined analysis technique for the search for fast magnetic monopoles with the MACRO detector / MACRO Collaboration
We describe a search method for fast moving ( beta = v/c > 5 * 10/sup -3/) magnetic monopoles using simultaneously the scintillator, streamer tube and track-etch subdetectors of the MACRO apparatus. The first two subdetectors are used primarily for the identification of candidates while the track-etch one is used as the final tool for their rejection or confirmation. [...]
2002 - Published in : Astropart. Phys. 18 (2002) 27-41
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8.
Neutrino oscillations at high energy by MACRO / MACRO Collaboration
INFN-AE-99-09. - 1999. - 4 p.
Fulltext - Fulltext
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9.
Muon Energy Estimate Through Multiple Scattering with the Macro Detector / MACRO Collaboration
Muon energy measurement represents an important issue for any experiment addressing neutrino induced upgoing muon studies. Since the neutrino oscillation probability depends on the neutrino energy, a measurement of the muon energy adds an important piece of information concerning the neutrino system. [...]
physics/0203018.- Bologna : Bologna Univ. INFN, 2002 - 25 p. - Published in : Nucl. Instrum. Methods Phys. Res., A 492 (2002) 376-386 Access to fulltext document: PDF; External link: physics/0203018 PDF
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10.
Matter effects in upward-going muons and sterile neutrino oscillations / MACRO Collaboration
The angular distribution of upward-going muons produced by atmospheric neutrinos in the rock below the MACRO detector shows anomalies in good agreement with two flavor nu /sub mu / to nu /sub tau / oscillations with maximum mixing and Delta m/sup 2/ around 0.0024 eV/sup 2/. Exploiting the dependence of magnitude of the matter effect on the oscillation channel, and using a set of 809 upward-going muons observed in MACRO, we show that the two flavor nu /sub mu / to nu /sub s/ oscillation is disfavored with 99% C.L. [...]
2001 - Published in : Phys. Lett. B 517 (2001) 59-66
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68 Vakili, M
3 Vakili, Mohammadjavad
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