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CERN Document Server 找到 117 笔记录  1 - 10下一个最後  跳到记录: 检索需时 0.52 秒. 
1.
A measurement of the decay K(L) ---> pi0 gamma gamma / Heinz, R (Mainz U., Inst. Phys.) /NA31
1992 - 4 p. - Published in : (1992) , pp. 177-180 Fulltext: PDF;
In : 27th Rencontres de Moriond : Leptonic Session, Les Arcs, France, 15 - 22 Mar 1992, pp.177-180
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2.
Experimental study of REACTIONS:P+P⇄π+d (combined report) / Chapman, K R ; Jones, T W ; Khan, Q H ; Mckee, J S C ; B , Van der Raay H ; Tanimura, Y ; Heinz, R M ; W , Jones L ; J , Longo M ; E , Overseth 0 et al.
4 p. - Published in : : 1, pp. 52-55 Published version: PDF;
In : 12th International Conference on High-energy Physics, v.1 (Eng.), Dubna, Soviet Union, 5 - 15 Aug 1964, pp.52-55
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3.
Possible observation of a meson at 5.3 GeV/c$^{2}$ / Barate, R (Saclay) ; Bareyre, P (Saclay) ; Bonamy, P (Saclay) ; Borgeaud, P (Saclay) ; David, M (Saclay) ; Ernwein, J (Saclay) ; Gentit, F X (Saclay) ; Laurens, G (Saclay) ; Lemoigne, Y (Saclay) ; Roussarie, A (Saclay) et al.
CERN-EP-79-113. - 1979. - 17 p.
Fulltext
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4.
High-mass muon pairs produced in $\pi{-}$Be collisions at 150 and 175 GeV/c / Abolins, M A (Saclay) ; Barate, R (Saclay) ; Bareyre, P (Saclay) ; Bonamy, P (Saclay) ; Borgeaud, P (Saclay) ; Brisson, J C (Saclay) ; David, M (Saclay) ; Ernwein, J (Saclay) ; Gentit, F X (Saclay) ; Laurens, G (Saclay) et al.
CERN-EP-79-69. - 8 p.
Fulltext
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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.
High transverse energy hadronic collisions at 400 GeV/c / E557 Collaboration
Large transverse momentum particles in hadron collisions are thought to arise from hard constituent scattering where the scattered constituents manifest themselves as jets of hadrons. Cross-sections for the production of narrow jets have been measured and found to agree with a simple quark-parton model. [...]
1982 - Published in : J. Phys. Colloq. 43 (1982) C3-127
In : 21st International Conference on High-energy Physics, Paris, France, 26 - 31 Jul 1982, pp.C3-127
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CERN Document Server : 找到 117 笔记录   1 - 10下一个最後  跳到记录:
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