L
L. Patrizii
Researcher at University of Bologna
Publications - 35
Citations - 577
L. Patrizii is an academic researcher from University of Bologna. The author has contributed to research in topics: Cosmic ray & Detector. The author has an hindex of 13, co-authored 35 publications receiving 538 citations.
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Journal ArticleDOI
Measurements of atmospheric muon neutrino oscillations, global analysis of the data collected with MACRO detector
M. Ambrosio,R. Antolini,D. Bakari,A. Baldini,G. C. Barbarino,B. C. Barish,G. Battistoni,Yvonne Becherini,Roberto Bellotti,C. Bemporad,P. Bernardini,Halina Bilokon,C. Bloise,C. R. Bower,M. Brigida,F. Cafagna,D. Campana,M. Carboni,S. Cecchini,S. Cecchini,Fabrizio Cei,V. Chiarella,B. C. Choudhary,D. Cosson,S. Coutu,G. de Cataldo,H. Dekhissi,C. De Marzo,I. De Mitri,U. Denni,J. Derkauoi,M. De Vincenzi,A. Di Credico,C. Favuzzi,C. Forti,A. Frani,P. Fusco,G. Giacomelli,G. Giannini,G. Giannini,N. Giglietto,M. Giorgini,M. Grassi,A. A. Grillo,F. Guarino,C. Gustavino,Alec Habig,Alec Habig,Kael Hanson,R.M. Heinz,E. Iarocci,E. Katsavounidis,E. Katsavounidis,Ioannis Katsavounidis,E. Kearns,Hyun-Chul Kim,S. Kyriazopoulou,E. Lamanna,E. Lamanna,C. E. Lane,D. Levin,Paolo Lipari,M. J. Longo,F. Loparco,F. Maaroufi,G. Mancarella,G. Mandrioli,Shahid Manzoor,Shahid Manzoor,Annarita Margiotta,Andrea Carlo Marini,D. Martello,A. Marzari-Chiesa,M. N. Mazziotta,A. Mengucci,D. G. Michael,S P Mikheyev,P. Monacelli,Teresa Montaruli,Marco Monteno,S. L. Mufson,J. A. Musser,Donato Nicolo,R. Nolty,C. Orth,Giuseppe Osteria,O. Palamara,Vincenzo Patera,L. Patrizii,R. Pazzi,C. W. Peck,L. Perrone,S. Petrera,V. Popa,A. Rainò,J. Reynoldson,Frederic Jean Ronga,C. Satriano,C. Satriano,Kate Scholberg,Kate Scholberg,A. Sciubba,Maximiliano Sioli,Mario Sitta,Mario Sitta,P. Spinelli,M. Spinetti,Maurizio Spurio,R. Steinberg,J. L. Stone,L. R. Sulak,A. Surdo,Gregory Tarle,V. Togo,M. Vakili,C. W. Walter,R. C. Webb +116 more
TL;DR: The final analysis of atmospheric neutrino events collected with the MACRO detector is presented in this article, where three different classes of events, generated by neutrinos in different energy ranges, are studied.
Journal ArticleDOI
Magnetic monopole search at high altitude with the SLIM experiment
S. Balestra,S. Cecchini,S. Cecchini,M. Cozzi,M. Errico,Fabrizio Fabbri,G. Giacomelli,R. Giacomelli,M. Giorgini,Ashavani Kumar,Ashavani Kumar,Shahid Manzoor,Shahid Manzoor,J. McDonald,G. Mandrioli,Stefano Marcellini,Annarita Margiotta,E. Medinaceli,E. Medinaceli,L. Patrizii,James Pinfold,V. Popa,I.E. Qureshi,O. Saavedra,Z. Sahnoun,G. Sirri,Maurizio Spurio,V. Togo,Antonio Velarde,A. Zanini +29 more
TL;DR: The SLIM experiment was a large array of nuclear track detectors located at the Chacaltaya high altitude Laboratory (5230m a.s.l.) as discussed by the authors, which was particularly sensitive to intermediate mass magnetic monopoles.
Journal ArticleDOI
Results of the search for strange quark matter and Q-balls with the SLIM experiment
S. Cecchini,S. Cecchini,M. Cozzi,D. Di Ferdinando,M. Errico,Fabrizio Fabbri,G. Giacomelli,R. Giacomelli,M. Giorgini,Ashavani Kumar,Ashavani Kumar,J. McDonald,G. Mandrioli,Shahid Manzoor,Shahid Manzoor,Annarita Margiotta,E. Medinaceli,E. Medinaceli,L. Patrizii,James Pinfold,V. Popa,I.E. Qureshi,O. Saavedra,Z. Sahnoun,G. Sirri,Maurizio Spurio,V. Togo,C. Valieri,Antonio Velarde,A. Zanini +29 more
TL;DR: The SLIM experiment at the Chacaltaya high altitude laboratory was sensitive to nuclearites and Q-balls which could be present in the cosmic radiation as possible Dark Matter components.
Journal ArticleDOI
Bulk etch rate measurements and calibrations of plastic nuclear track detectors
S. Balestra,M. Cozzi,G. Giacomelli,R. Giacomelli,M. Giorgini,Ashavani Kumar,Ashavani Kumar,G. Mandrioli,Shahid Manzoor,Shahid Manzoor,Annarita Margiotta,E. Medinaceli,L. Patrizii,V. Popa,I.E. Qureshi,Mukhtar Ahmed Rana,G. Sirri,Maurizio Spurio,V. Togo,C. Valieri +19 more
TL;DR: In this article, a new method for the bulk etch rate determination, using both cone height and base diameter measurements, was developed, which was used for the detection of nuclear fragments.
Journal ArticleDOI
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
Marco Aglietta,Bruno Alessandro,Pietro Antonioli,F. Arneodo,L. Bergamasco,M. E. Bertaina,Carlotta Castagnoli,Antonella Castellina,A. Chiavassa,G. Cini,B. D'Ettorre Piazzoli,G. Di Sciascio,W. Fulgione,P. Galeotti,P. L. Ghia,M. Iacovacci,G. Mannocchi,C. Morello,G. Navarra,O. Saavedra,A. Stamerra,A. Stamerra,G. C. Trinchero,S. Valchierotti,P. Vallania,S. Vernetto,Carlo Vigorito,M. Ambrosio,R. Antolini,A. Baldini,G. C. Barbarino,B. C. Barish,G. Battistoni,Yvonne Becherini,Roberto Bellotti,C. Bemporad,P. Bernardini,Halina Bilokon,C. R. Bower,M. Brigida,Severino Angelo Maria Bussino,F. Cafagna,M. Calicchio,D. Campana,M. Carboni,R. Caruso,S. Cecchini,S. Cecchini,Fabrizio Cei,V. Chiarella,Tommaso Chiarusi,B. C. Choudhary,S. Coutu,S. Coutu,M. Cozzi,G. de Cataldo,H. Dekhissi,C. De Marzo,I. De Mitri,J. Derkaoui,M. De Vincenzi,A. Di Credico,O. Erriquez,C. Favuzzi,C. Forti,P. Fusco,G. Giacomelli,G. Giannini,G. Giannini,N. Giglietto,M. Giorgini,M. Grassi,A. A. Grillo,F. Guarino,C. Gustavino,Alec Habig,Alec Habig,Kael Hanson,R.M. Heinz,E. Iarocci,E. Katsavounidis,E. Katsavounidis,Ioannis Katsavounidis,E. Kearns,Hyun-Chul Kim,S. Kyriazopoulou,E. Lamanna,E. Lamanna,C. E. Lane,D. Levin,Paolo Lipari,Np Longley,Np Longley,M. J. Longo,F. Loparco,F. Maaroufi,G. Mancarella,G. Mandrioli,Annarita Margiotta,Andrea Carlo Marini,D. Martello,A. Marzari-Chiesa,M. N. Mazziotta,D. G. Michael,P. Monacelli,Teresa Montaruli,Marco Monteno,S. L. Mufson,J. A. Musser,Donato Nicolo,R. Nolty,C. Orth,Giuseppe Osteria,O. Palamara,Vincenzo Patera,L. Patrizii,R. Pazzi,C. W. Peck,L. Perrone,S. Petrera,V. Popa,A. Rainò,J. Reynoldson,F.J. Ronga,C. Satriano,C. Satriano,Eugenio Scapparone,Kate Scholberg,Kate Scholberg,A. Sciubba,Maximiliano Sioli,G. Sirri,Mario Sitta,Mario Sitta,P. Spinelli,M. Spinetti,Maurizio Spurio,R. Steinberg,J. L. Stone,L. R. Sulak,A. Surdo,Gregory Tarle,V. Togo,M. Vakili,C. W. Walter,R. C. Webb +145 more
TL;DR: In this paper, 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.l.).