L. Cifarelli
University of Bologna
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Featured researches published by L. Cifarelli.
Physics Letters B | 1992
M. Derrick; D. Krakauer; S. Magill; B. Musgrave; J. Repond; K. Sugano; R. W. Stanek; R. L. Talaga; J. L. Thron; F. Arzarello; R. Ayed; G. Barbagli; G. Bari; M. Basile; L. Bellagamba; D. Boscherini; G. Bruni; P. Bruni; Gc Romeo; G. Castellini; M. Chiarini; L. Cifarelli; F. Cindolo; F. Ciralli; A. Contin; S. D'Auria; C. Del Papa; F. Frasconi; P. Giusti; G. Iacobucci
Abstract The total photoproduction cross section is determined from a measurement of electroproduction with the ZEUS detector at HERA. The Q 2 values of the virtual photons are in the range 10 −7 Q 2 −2 GeV 2 . The γp total cross section in the γp centre of mass energy range 186–233 GeV is 154 ± 16 (stat.) ± 32 (syst.) μ b.
Physical Review D | 1998
M. Aglietta; B. Alpat; E. D. Alyea; P. Antonioli; G. Badino; G. Bari; M. Basile; V. S. Berezinsky; F. Bersani; M. Bertaina; R. Bertoni; G. Bonoli; A. Bosco; G. Bruni; G. Cara Romeo; C. Castagnoli; A. Castellina; A. Chiavassa; J. Chinellato; L. Cifarelli; F. Cindolo; G. Conforto; A. Contin; V. L. Dadykin; A. De Silva; M. Deutsch; P. Dominici; L. G. Dos Santos; L. Emaldi; R. I. Enikeev
We present the analysis of the muon events with all muon multiplicities collected during 21804 hours of operation of the first LVD tower. The measured angular distribution of muon intensity has been converted to the `depth -- vertical intensity relation in the depth range from 3 to 12 km w.e.. The analysis of this relation allowed to derive the power index,
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2002
A. Akindinov; A. Alici; F. Anselmo; P. Antonioli; Y.W. Baek; M. Basile; G. Cara Romeo; E. Cerron-Zeballos; L. Cifarelli; F. Cindolo; A. De Caro; S. De Pasquale; A. Di Bartolomeo; M. Fusco Girard; M. Guida; D. Hatzifotiadou; S.M. Kisselev; G. Laurenti; M.L. Luvisetto; A. Margotti; A.N. Martemiyanov; S.V. Morozov; R. Nania; A. Pesci; F. Pierella; G. Scioli; S. Sellitto; A.V. Smirnitski; G. Valenti; D. Vicinanza
gamma
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1999
D Alvisi; F Anselmo; L. Baldini; G. Bari; M. Basile; L. Bellagamba; A. Bruni; G. Bruni; D. Boscherini; D. Casadei; G. Cara Romeo; G. Castellini; L. Cifarelli; F. Cindolo; A. Contin; S. De Pasquale; P. Giusti; G. Iacobucci; G. Laurenti; G. Levi; A. Margotti; T. Massam; R. Nania; F. Palmonari; A. Polini; S Recupero; G. Sartorelli; C. Williams; A. Zichichi
, of the primary all-nucleon spectrum:
Physical Review D | 1999
M. Aglietta; B. Alpat; E. D. Alyea; P. Antonioli; G. Badino; G. Bari; M. Basile; V. S. Berezinsky; F. Bersani; M. Bertaina; R. Bertoni; G. Bonoli; A. Bosco; G. Bruni; G. Cara Romeo; C. Castagnoli; A. Castellina; A. Chiavassa; J. Chinellato; L. Cifarelli; F. Cindolo; G. Conforto; A. Contin; V. L. Dadykin; A. De Silva; M. Deutsch; P. Dominici; L. G. Dos Santos; L. Emaldi; R. I. Enikeev
gamma=2.78 pm 0.05
Journal of Instrumentation | 2014
D. De Gruttola; M. Abbrescia; A. Agocs; S. Aiola; R. Antolini; C. Avanzini; R. Baldini Ferroli; G. Bencivenni; E. Bossini; E. Bressan; A. Chiavassa; C. Cicalò; L. Cifarelli; E. Coccia; S. De Pasquale; A. Di Giovanni; M. D'Incecco; M. Dreucci; F.L. Fabbri; V. Frolov; M. Garbini; G. Gemme; I. Gnesi; C. Gustavino; D. Hatzifotiadou; P. La Rocca; S. Li; F. Librizzi; A. Maggiora; M. Massai
. The `depth -- vertical intensity relation has been converted to standard rock and the comparison with the data of other experiments has been done. We present also the derived vertical muon spectrum at sea level.
Journal of Instrumentation | 2016
P. La Rocca; M. Abbrescia; C. Avanzini; L. Baldini; R. Baldini Ferroli; G. Batignani; G. Bencivenni; E. Bossini; A. Chiavassa; C. Cicalò; L. Cifarelli; F. Coccetti; E. Coccia; A. Corvaglia; D. De Gruttola; S. De Pasquale; A. Di Giovanni; M. D'Incecco; M. Dreucci; F.L. Fabbri; E. Fattibene; A. Ferraro; Vladimir Frolov; P. Galeotti; M. Garbini; G. Gemme; I. Gnesi; S. Grazzi; C. Gustavino; D. Hatzifotiadou
Abstract The selected device for the ALICE Time-of-Flight array is the Multigap Resistive Plate Chamber (MRPC). We have tested this device at the Gamma Irradiation Facility at CERN to evaluate the rate dependence. We find that the rate capability of the MRPC easily exceeds the 50 Hz/cm 2 maximum expected rate at the ALICE experiment. In addition, we have measured the power dissipated for an equivalent flux of 1.6 kHz/cm 2 of through-going muons to be 650 mW/m 2 .
14th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2015 | 2016
M. Abbrescia; C. Avanzini; L. Baldini; R. Baldini Ferroli; G. Batignani; G. Bencivenni; E. Bossini; E. Bressan; A Chiavassa; C. Cicalò; L. Cifarelli; E. Coccia; A. Corvaglia; D. De Gruttola; S. De Pasquale; A. Di Giovanni; M. D’Incecco; M. Dreucci; F.L. Fabbri; E. Fattibene; A Ferrarov; R. Forster; V. Frolov; P. Galeotti; M. Garbini; G. Gemme; I. Gnesi; S. Grazzi; C. Gustavino; D. Hatzifotiadou
The system of plastic scintillator counters for the AMS experiment is described. The main characteristics of the detector are: (a) large sensitive area (four 1.6 m2 planes) with small dead space; (b) low-power consumption (150 W for the power and the read-out electronics of 336 PMs); (c) 120 ps time resolution. ( 1999 Elsevier Science B.V. All rights reserved.
ieee nuclear science symposium | 2009
M. Abbrescia; A. Alici; S. An; R. Antolini; A. Badalà; Y. W. Baek; R. Baldini Ferroli; G. Bencivenni; F. Blanco; E. Bressan; A. Chiavassa; C. Chiri; C. Cicalò; L. Cifarelli; F. Coccetti; A. De Carom; D. De Gruttola; S. De Pasquale; M. D'Incecco; F.L. Fabbri; V. Frolov; M. Garbini; C. Guarnaccia; C. Gustavino; D. Hatzifotiadou; J. S. Kim; M.M. Kim; P. La Rocca; F. Librizzi; A. Maggiora
We present the analysis of the muon events with all muon multiplicities collected during 21804 hours of operation of the first LVD tower. The measured depth-angular distribution of muon intensities has been used to obtain the normalization factor, A, the power index, gamma, of the primary all-nucleon spectrum and the ratio, R_c, of prompt muon flux to that of pi-mesons - the main parameters which determine the spectrum of cosmic ray muons at the sea level. The value of gamma = 2.77 +/- 0.05 (68% C.L.) and R_c<2.0 x 10^-3 (95% C.L.) have been obtained. The upper limit to the prompt muon flux favours the models of charm production based on QGSM and the dual parton model.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2004
A. Akindinov; A. Alici; F. Anselmo; P. Antonioli; M. Basile; G. Cara Romeo; L. Cifarelli; F. Cindolo; F. Cosenza; I. D'Antone; A. De Caro; S. De Pasquale; A. Di Bartolomeo; M. Fusco Girard; V. Golovine; M. Guerzoni; M. Guida; D. Hatzifotiadou; A.B. Kaidalov; Doojin Kim; D. W. Kim; S.M. Kisselev; G. Laurenti; K. S. Lee; S. Lee; E. Lioublev; M.L. Luvisetto; A. Margotti; A.N. Martemiyanov; F. Massera
The Extreme Energy Events (EEE) Project is a Centro Fermi - CERN - INFN - MIUR Collaboration Project for the study of extremely high energy cosmic rays, which exploits the Multigap Resistive Plate Chamber (MRPC) technology. The excellent time resolution and good tracking capability of this kind of detector allows us to study Extensive Air Showers (EAS) with an array of MRPC telescopes distributed across the Italian territory. Each telescope is installed in a high school, with the further goal to introduce students to particle and astroparticle Physics. The status of the experiment and the results obtained are reported.