E
E. Vannuccini
Researcher at Istituto Nazionale di Fisica Nucleare
Publications - Â 22
Citations - Â 1719
E. Vannuccini is an academic researcher from Istituto Nazionale di Fisica Nucleare. The author has contributed to research in topics: Cosmic ray & Isotopes of helium. The author has an hindex of 14, co-authored 22 publications receiving 1581 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
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.
Journal ArticleDOI
Status of the GAMMA-400 Project
A. M. Galper,A. M. Galper,O. Adriani,R. L. Aptekar,I. V. Arkhangelskaja,A.I. Arkhangelskiy,Mirko Boezio,V. Bonvicini,K. A. Boyarchuk,Yu. V. Gusakov,M. O. Farber,M. I. Fradkin,V. A. Kachanov,Vladimir Kaplin,M. D. Kheymits,A. A. Leonov,Francesco Longo,Paolo Maestro,P S Marrocchesi,E. P. Mazets,E. Mocchiutti,A. A. Moiseev,Nicola Mori,Igor V. Moskalenko,P. Yu. Naumov,P. Papini,P. Picozza,V. G. Rodin,M. F. Runtso,Roberta Sparvoli,Piero Spillantini,S. I. Suchkov,Marco Tavani,N. P. Topchiev,Andrea Vacchi,E. Vannuccini,Yu. T. Yurkin,N. Zampa,V. G. Zverev +38 more
TL;DR: In this paper, the preliminary design of the new space gamma-ray telescope GAMMA-400 for the energy range 100 MeV-3 TeV is presented, which is optimized to address a broad range of science topics, such as search for signatures of dark matter, studies of galactic and extragalactic gamma-rays sources, Galactic and extrgalactic diffuse emission, gamma burst, as well as high-precision measurements of spectra of cosmic-ray electrons, positrons, and nuclei.
Journal ArticleDOI
The discovery of geomagnetically trapped cosmic ray antiprotons
O. Adriani,Giancarlo Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,Massimo Bongi,V. Bonvicini,S. Borisov,S. 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. Grishantseva,G. Jerse,A. V. Karelin,M. D. Kheymits,Sergey Koldashov,S. Y. Krutkov,A. N. Kvashnin,Alexey Leonov,V. V. Malakhov,L. Marcelli,A. G. Mayorov,W. Menn,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,N. N. Nikonov,Giuseppe Osteria,F. Palma,Paolo Papini,Mark Pearce,P. Picozza,C. Pizzolotto,M. Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,M. Simon,Roberta Sparvoli,Piero Spillantini,Yuri Stozhkov,Andrea Vacchi,E. Vannuccini,G. Vasilyev,S. A. Voronov,Y. T. Yurkin,Juan Wu,Juan Wu,Gianluigi Zampa,N. Zampa,V. G. Zverev +65 more
TL;DR: The existence of a significant flux of antiprotons confined to Earth's magnetosphere has been considered in several theoretical works as discussed by the authors, which constitutes the main source of trapped protons at energies above some tens of MeV.