R
R. Carbone
Researcher at University of Rome Tor Vergata
Publications - Â 33
Citations - Â 1987
R. Carbone is an academic researcher from University of Rome Tor Vergata. The author has contributed to research in topics: Cosmic ray & PAMELA detector. The author has an hindex of 15, co-authored 33 publications receiving 1855 citations.
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Journal ArticleDOI
PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra
O. Adriani,O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,Lorenzo Bonechi,M. Bongi,V. Bonvicini,S. V. Borisov,S. Bottai,A. Bruno,F. Cafagna,D. Campana,R. Carbone,Per Carlson,Marco Casolino,G. Castellini,L. Consiglio,M. P. De Pascale,C. De Santis,N. De Simone,V. Di Felice,A. M. Galper,William Gillard,L. A. Grishantseva,Giovanna Jerse,A. V. Karelin,S. V. Koldashov,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,V. Malvezzi,L. Marcelli,A. G. Mayorov,W. Menn,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,Nicola Mori,N. N. Nikonov,G. Osteria,F. Palma,P. Papini,Mark Pearce,P. Picozza,C. Pizzolotto,Marco Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,M. Simon,Roberta Sparvoli,P. Spillantini,P. Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Y. T. Yurkin,Juan Wu,G. Zampa,N. Zampa,V. G. Zverev +68 more
TL;DR: PAMELA data challenge the current paradigm of cosmic-ray acceleration in supernova remnants followed by diffusive propagation in the Galaxy and find that the spectral shapes of these two species are different and cannot be described well by a single power law.
Journal ArticleDOI
A statistical procedure for the identification of positrons in the PAMELA experiment
O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,M. Bongi,V. Bonvicini,S. V. Borisov,S. Bottai,A. Bruno,F. Cafagna,D. Campana,R. Carbone,Per Carlson,Marco Casolino,G. Castellini,L. Consiglio,M. P. De Pascale,C. De Santis,N. De Simone,V. Di Felice,A. M. Galper,William Gillard,L. A. Grishantseva,Petter Hofverberg,Giovanna Jerse,S. V. Koldashov,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. Malvezzi,L. Marcelli,W. Menn,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,N. N. Nikonov,G. Osteria,P. Papini,Mark Pearce,P. Picozza,Marco Ricci,S. B. Ricciarini,Laura Rossetto,M. Simon,Roberta Sparvoli,Piero Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Juan Wu,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev,Domenico Marinucci +60 more
TL;DR: The PAMELA satellite experiment has measured the cosmic-ray positron fraction between 1.5 GeV and 100 GeV, and the need to reliably discriminate between the positron signal and proton background has required the development of an ad hoc analysis procedure.
Journal ArticleDOI
Measurement of the Flux of Primary Cosmic Ray Antiprotons with Energies of 60 MeV to 350 GeV in the PAMELA Experiment
O. Adriani,G. A. Bazilevskaya,G. C. Barbarino,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,V. Bonvicini,M. Bongi,Lorenzo Bonechi,S. V. Borisov,S. V. Borisov,S. Bottai,A. Bruno,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Juan Wu,A. M. Galper,L. A. Grishantseva,I. A. Danilchenko,William Gillard,Giovanna Jerse,G. Zampa,N. Zampa,V. G. Zverev,Marco Casolino,D. Campana,R. Carbone,A. V. Karelin,Per Carlson,G. Castellini,F. Cafagna,A. N. Kvashnin,S. V. Koldashov,Sergey Koldobskiy,S. Y. Krutkov,L. Consiglio,A. A. Leonov,A. G. Mayorov,V. V. Malakhov,W. Malvezzi,L. Marcelli,W. Menn,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,N. N. Nikonov,N. N. Nikonov,G. Osteria,F. Palma,P. Papini,C. Pizzolotto,M. P. De Pascale,P. Picozza,Mark Pearce,Marco Ricci,S. B. Ricciarini,Laura Rossetto,M. F. Runtso,C. De Santis,Ritabrata Sarkar,M. Simon,N. De Simone,Roberta Sparvoli,P. Spillantini,Yuri Stozhkov,V. Di Felice,Y. T. Yurkin +69 more
TL;DR: In this paper, the antiproton spectrum and the ratio of the fluxes of primary cosmic ray antiprotons to protons with energies of 60 MeV to 350 GeV were measured from the data obtained from June 2006 to January 2010 in the PAMELA experiment.
Journal ArticleDOI
Measurement of Boron and Carbon Fluxes in Cosmic Rays with the PAMELA Experiment
O. Adriani,Giancarlo Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,Massimo Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,R. Carbone,Per Carlson,Marco Casolino,G. Castellini,I. A. Danilchenko,C. De Donato,C. De Santis,N. De Simone,V. Di Felice,Valerio Formato,A. M. Galper,A. V. Karelin,Sergey Koldashov,Sergey Koldobskiy,S. Y. Krutkov,A. N. Kvashnin,Alexey Leonov,V. V. Malakhov,L. Marcelli,M. Martucci,A. G. Mayorov,W. Menn,M. Merge,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,R. Munini,Giuseppe Osteria,F. Palma,B. Panico,Paolo Papini,Mark Pearce,P. Picozza,C. Pizzolotto,M. Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,V. Scotti,M. Simon,Roberta Sparvoli,Piero Spillantini,Yuri Stozhkov,Andrea Vacchi,E. Vannuccini,G. Vasilyev,S. A. Voronov,Y. T. Yurkin,Gianluigi Zampa,N. Zampa,V. G. Zverev +63 more
TL;DR: In this article, the absolute fluxes of boron and carbon nuclei as well as the B/C ratio from the PAMELA space experiment were measured for data taken in the period 2006 July to 2008 March.
Journal ArticleDOI
Measurement of boron and carbon fluxes in cosmic rays with the PAMELA experiment
O. Adriani,Giancarlo Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,Massimo Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,R. Carbone,Per Carlson,Marco Casolino,G. Castellini,I. A. Danilchenko,C. De Donato,C. De Santis,N. De Simone,V. Di Felice,Valerio Formato,A. M. Galper,A. V. Karelin,Sergey Koldashov,Sergey Koldobskiy,S. Y. Krutkov,A. N. Kvashnin,Alexey Leonov,V. V. Malakhov,L. Marcelli,M. Martucci,A. G. Mayorov,W. Menn,M. Merge,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,R. Munini,Giuseppe Osteria,F. Palma,B. Panico,Paolo Papini,Mark Pearce,P. Picozza,C. Pizzolotto,M. Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,V. Scotti,M. Simon,Roberta Sparvoli,Piero Spillantini,Yuri Stozhkov,Andrea Vacchi,E. Vannuccini,G. Vasilyev,S. A. Voronov,Y. T. Yurkin,Gianluigi Zampa,N. Zampa,V. G. Zverev +63 more
TL;DR: In this article, the absolute fluxes of boron and carbon nuclei, as well as the B/C ratio, from the PAMELA space experiment were investigated.