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CERN Document Server Sök i 57 journaler efter:  1 - 10nästaslut  gå till journal: Sökningen tog 0.61 sekunder. 
1.
The CMS experiment at the CERN LHC / CMS Collaboration
2008 - 361 p. - Published in : JINST 3 (2008) S08004 SISSA/IOP Open Access article: PDF;
In : The CERN Large Hadron Collider - Please contact the library if you need to access this document.
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2.
Search for SUSY in Final States with Z Bosons / Kyriazopoulou, Sophia ; Markou, Christos
A search for SUSY processes leading to final states with Z bosons is performed at a low mass point in the mSUGRA parameter space. The signature of such processes is studied using both a complete and a fast simulation. [...]
CMS-NOTE-2006-116.- Geneva : CERN, 2006 - 14 p. Fulltext: PDF;
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3.
CMS Physics : Technical Design Report Volume 2: Physics Performance / Bayatian, G L
CERN-LHCC-2006-021 CMS-TDR-8-2. - Geneva : CERN, 2007. - 669 p. (Technical design report. CMS ; 8.2)


10.1088/0954-3899/34/6/S01
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4.
CMS Physics : Technical Design Report Volume 1: Detector Performance and Software / Bayatian, G L
CERN-LHCC-2006-001 CMS-TDR-8-1. - Geneva : CERN, 2006. - 521 p. (Technical design report. CMS ; 8.1)

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5.
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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6.
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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7.
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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8.
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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9.
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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10.
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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CERN Document Server : Sök i 57 journaler efter:   1 - 10nästaslut  gå till journal:
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1 Kyriazopoulou, S.
2 Kyriazopoulou, Sophia
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