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Featured researches published by A. Bosco.


Physical Review D | 1998

Muon ''depth-intensity'' relation measured by the LVD underground experiment and cosmic-ray muon spectrum at sea level

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,


Physical Review D | 1999

Upper limit on the prompt muon flux derived from the LVD underground experiment

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


Archive | 1997

Search for point sources with muons observed by LVD

Massimo Aglietta; B. Alpat; E. D. Alyea; P. Antonioli; G. Badino; G. Bari; Maurizio Basile; Veniamin Sergeevich Berezinsky; F. Bersani; M. Bertaina; Roberto Bertoni; G. Bonoli; A. Bosco; G. Bruni; Giovanni Romeo; C. Castagnoli; Antonella Castellina; A. Chiavassa; J. Chinellato; Luisa 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

, of the primary all-nucleon spectrum:


Archive | 1997

Upper limit on the prompt muon flux derived from the LVD data

Massimo Aglietta; B. Alpat; E. D. Alyea; P. Antonioli; G. Badino; G. Bari; Maurizio Basile; Veniamin Sergeevich Berezinsky; F. Bersani; M. Bertaina; Roberto Bertoni; G. Bonoli; A. Bosco; G. Bruni; Giovanni Romeo; C. Castagnoli; Antonella Castellina; A. Chiavassa; J. Chinellato; Luisa 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


Archive | 1997

An energy signature for very deep underground muons observed by the LVD experiment

Massimo Aglietta; B. Alpat; E. D. Alyea; P. Antonioli; G. Badino; G. Bari; Maurizio Basile; Veniamin Sergeevich Berezinsky; F. Bersani; M. Bertaina; Roberto Bertoni; G. Bonoli; A. Bosco; G. Bruni; Giovanni Romeo; C. Castagnoli; Antonella Castellina; A. Chiavassa; J. Chinellato; Luisa 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

. 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.


Contributed to | 1997

Study of neutrinos from stellar collapses with the LVD experiment in the Gran Sasso Laboratory

M. Aglietta; V. S. Berezinsky; F. Bersani; P. Galeotti; G. Bonoli; I. Uman; V.G. Ryasnii; Taizo Wada; L. Cifarelli; G.C. Trinchero; O. G. Ryazhskaya; I. A. Pless; K. Lau; V. F. Yakushev; S. Vernetto; E. Hafen; C. Melagrana; P. V. Korchagin; A. S. Malguin; M. Widgoff; L. Periale; E. von Goeler; P. L. Ghia; P. Haridas; L. Pinsky; N. Taborgna; G. Conforto; G. Bruni; R. Weinstein; M. Basile

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.


Bulletin of The Russian Academy of Sciences: Physics | 1997

STUDYING ENERGETIC MUONS AT THE LVD SETUP

M. Aglietta; B. Alpat; E. D. Alyea; P. Antonioli; G. Badino; G. Bari; M. Basile; V. S. Berezinsky; M. Bertaina; R. Bertoni; A. Bosco; G. Bruni; Giovanni Romeo; K. Castagnoli; A. Castellina; A. Ciavassa; D. A. Cinellato; L. Cifarelli; F. Cindalo; D. Conforto; A. Contin; V. L. Dadykin; S. De Paskuale; P. Deziati; A. De Silva; M. Deutsch; P. Dominici; L. G. Dos Santos; R. I. Enikeev; F. Fabbri


Archive | 1994

The depth-intensity distribution of single and double muon events measured by the LVD underground experiment in the Gran Sasso laboratory

M. Aglietta; V. S. Berezinsky; X. Zhu; G. Maccarrone; Taizo Wada; I. Uman; R. Casaccia; G.C. Trinchero; O. G. Ryazhskaya; I. A. Pless; K. Lau; V. F. Yakushev; G. Brugnola; S. Vernetto; L. Bergamasco; S. Wang; M. Widgoff; L. Periale; H. Wang; A. Zallo; E. von Goeler; L. Pinsky; D. Shen; F. Wang; G. Bruni; R. Weinstein; Y. Bans; M. Basile; P. Antonioli; D. Sanders

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G. Bruni

University of Bologna

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P. Antonioli

Istituto Nazionale di Fisica Nucleare

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A. Contin

University of Bologna

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B. Alpat

University of Perugia

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G. Bari

University of Bologna

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G. Bonoli

University of Bologna

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G. Conforto

University of Florence

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