M. P. De Pascale
University of Rome Tor Vergata
213 Papers
1.3K Citations
M. P. De Pascale 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 39, co-authored 210 publications. Previous affiliations of M. P. De Pascale include Istituto Nazionale di Fisica Nucleare & INAF.
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Papers
An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV
O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,M. Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,Per Carlson,Marco Casolino,G. Castellini,M. P. De Pascale,G. De Rosa,N. De Simone,V. Di Felice,A. M. Galper,L. A. Grishantseva,Petter Hofverberg,S. V. Koldashov,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. Malvezzi,L. Marcelli,W. Menn,V. V. Mikhailov,E. Mocchiutti,Silvio Orsi,G. Osteria,P. Papini,Mark Pearce,P. Picozza,Marco Ricci,S. B. Ricciarini,M. Simon,Roberta Sparvoli,Piero Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev +50 more
TL;DR: It is found that the positron fraction increases sharply over much of that range, in a way that appears to be completely inconsistent with secondary sources, and is concluded that a primary source, be it an astrophysical object or dark matter annihilation, is necessary.
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.
Cosmic-Ray Electron Flux Measured by the PAMELA Experiment between 1 and 625 GeV
O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,Mirko Boezio,E. A. Bogomolov,M. Bongi,V. Bonvicini,S. V. Borisov,S. Bottai,A. Bruno,F. Cafagna,D. Campana,R. Carbone,P. 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,André Monaco,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,Piero Spillantini,Steven Stochaj,J. C. Stockton,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 +65 more
TL;DR: New results regarding negatively charged electrons between 1 and 625 GeV performed by the satellite-borne experiment PAMELA are presented, this is the first time that cosmic-ray e⁻ have been identified above 50 GeV.
PAMELA - A Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics
P. Picozza,A. M. Galper,G. Castellini,O. Adriani,F. Altamura,M. Ambriola,G. C. Barbarino,A. Basili,G. A. Bazilevskaja,R. Bencardino,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,M. Bongi,L. Bongiorno,V. Bonvicini,F. Cafagna,D. Campana,P. Carlson,Marco Casolino,C. De Marzo,M. P. De Pascale,G. De Rosa,D. Fedele,Petter Hofverberg,S. V. Koldashov,S. Yu. Krutkov,A. N. Kvashnin,J. Lund,J. Lundquist,O. Maksumov,V. Malvezzi,L. Marcelli,W. Menn,V. V. Mikhailov,M. Minori,S. Misin,E. Mocchiutti,A. Morselli,N. N. Nikonov,S. Orsi,Giuseppe Osteria,P. Papini,Mark Pearce,Marco Ricci,S. B. Ricciarini,M. F. Runtso,S. Russo,M. Simon,Roberta Sparvoli,Piero Spillantini,Yu. I. Stozhkov,E. Taddei,Andrea Vacchi,E. Vannuccini,S. A. Voronov,Y. T. Yurkin,Gianluigi Zampa,N. Zampa,V. G. Zverev +59 more
TL;DR: The PAMELA experiment is a satellite-borne apparatus designed to study charged particles in the cosmic radiation with a particular focus on antiparticles as discussed by the authors, which is mounted on the Resurs DK1 satellite that was launched from the Baikonur cosmodrome on June 15th 2006.
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An evaluation of the exposure in nadir observation of the JEM-EUSO mission
James H. Adams,Shafqat Ahmad,J. N. Albert,D. Allard,M. Ambrosio,Luis A. Anchordoqui,A. Anzalone,Y. Arai,C. Aramo,Katsuaki Asano,M. Ave,Pierre Barrillon,T. Batsch,J. Bayer,Tomás Belenguer,Roberto Bellotti,Andreas A. Berlind,M. E. Bertaina,M. E. Bertaina,P. L. Biermann,S. Biktemerova,C. Blaksley,J. Błe¸cki,S. Blin-Bondil,J. Blümer,Pavol Bobik,M. Bogomilov,Massimiliano Bonamente,Michael S. Briggs,Susana Briz,A. Bruno,F. Cafagna,D. Campana,J.N. Capdevielle,Rossella Caruso,Marco Casolino,Marco Casolino,Claudio Cassardo,Claudio Cassardo,G. Castellini,Osvaldo Catalano,Alberto Cellino,Michiyuki Chikawa,Mark Christl,Valerie Connaughton,J. F. Cortes,H. J. Crawford,R. Cremonini,S. Csorna,Juan Carlos D'Olivo,S. Dagoret-Campagne,A. J. de Castro,C. De Donato,C. De Donato,C. De La Taille,L. del Peral,A. Dell’Oro,M. P. De Pascale,M. P. De Pascale,M. Di Martino,G. Distratis,M. Dupieux,A. Ebersoldt,Toshikazu Ebisuzaki,Ralph Engel,S. Falk,Ke Fang,Francesco Fenu,I. Fernández-Gómez,Silvia Ferrarese,Silvia Ferrarese,A. Franceschi,J. Fujimoto,P. Galeotti,P. Galeotti,Gali Garipov,J. Geary,U.G. Giaccari,G. Giraudo,Maxim Gonchar,C. González Alvarado,P. Gorodetzky,Fausto Guarino,A. Guzmán,Y. Hachisu,B. Harlov,A. Haungs,J. Hernández Carretero,K. Higashide,T. Iguchi,H. Ikeda,N. Inoue,Susumu Inoue,A. Insolia,Francesco Isgrò,Yoshitaka Itow,E. Joven,E. G. Judd,A. Jung,F. Kajino,Toshitaka Kajino,I. Kaneko,Y. Karadzhov,J. Karczmarczyk,K. Katahira,K. Kawai,Yoshiya Kawasaki,B. Keilhauer,B. A. Khrenov,Jeong-Sook Kim,Soon-Wook Kim,Sug-Whan Kim,M. Kleifges,Pavel Klimov,Seung Hwan Ko,D. Kolev,I. Kreykenbohm,K. Kudela,Yoshimasa Kurihara,E. Kuznetsov,G. La Rosa,J. K. Lee,Javier Licandro,H. Lim,Fernando López,M. C. Maccarone,Karl Mannheim,L. Marcelli,L. Marcelli,A. Marini,G. Martin-Chassard,O. Martinez,G. Masciantonio,G. Masciantonio,K. Mase,R. Matev,A. Maurissen,G. Medina-Tanco,T. Mernik,H. Miyamoto,Y. Miyazaki,Yoshihiko Mizumoto,G. Modestino,D. Monnier-Ragaigne,J. A. Morales de los Ríos,B. Mot,T. Murakami,M. Nagano,M. Nagata,Shigehiro Nagataki,T. Nakamura,J. W. Nam,S. W. Nam,K. Nam,T. Napolitano,Dmitry V. Naumov,Andrii Neronov,Ken'ichi Nomoto,T. Ogawa,Hitoshi Ohmori,Angela V. Olinto,Piotr Orleanski,G. Osteria,N. Pacheco,M. I. Panasyuk,E. Parizot,Inkyu Park,B. Pastirčák,T. Patzak,T. Paul,C. Pennypacker,T. Peter,P. Picozza,P. Picozza,A. Pollini,H. Prieto,H. Prieto,Patrick J. Reardon,M. Reina,M. Reyes,M. Ricci,I. Rodríguez,M. D. Rodríguez Frías,Frederic Jean Ronga,Hanna Rothkaehl,G. Roudil,I. Rusinov,M. Rybczyński,M. D. Sabau,G. Sáez Cano,Akinori Saito,N. Sakaki,M. Sakata,Humberto Ibarguen Salazar,S. Sánchez,Andrea Santangelo,L. Santiago Crúz,M. Sanz Palomino,O. A. Saprykin,F. Sarazin,H. Sato,Mitsuteru Sato,Thomas Schanz,H. Schieler,Valentina Scotti,Mario Scuderi,A. Segreto,S. Selmane,Dmitri Semikoz,M. Serra,Sergei A. Sharakin,T. Shibata,Hirohiko M. Shimizu,K. Shinozaki,T. Shirahama,G. Siemieniec-Ozie¸bło,H. H. Silva Lopez,J. Sledd,K. Słomińska,A. Sobey,T. Sugiyama,D. Supanitsky,M. Suzuki,Barbara Szabelska,J. Szabelski,F. Tajima,N. Tajima,Toshiki Tajima,Yukihiro Takahashi,Hajime Takami,M. Takeda,Y. Takizawa,C. Tenzer,O. Tibolla,L. G. Tkachev,Taka Tomida,N. Tone,Frederic Trillaud,R. Tsenov,Katsuhiko Tsuno,T. Tymieniecka,Y. Uchihori,Ovidiu Vaduvescu,J. F. Valdés-Galicia,Piero Vallania,L. Valore,G. Vankova,Carlo Vigorito,Carlo Vigorito,L. Villaseñor,P. von Ballmoos,Satoshi Wada,J. Watanabe,Shigeto Watanabe,J. Watts,Marc Weber,Thomas J. Weiler,Tadeusz Wibig,L. R. Wiencke,M. Wille,Jörn Wilms,Z. Włodarczyk,Tokonatsu Yamamoto,Y. Yamamoto,Jianyi Yang,Hajime Yano,I. V. Yashin,Daisuke Yonetoku,K. Yoshida,S. Yoshida,R. Young,A. Zamora,A. Zuccaro Marchi +272 more
TL;DR: In this article, the authors evaluate the exposure during nadir observations with JEM-EUSO, the Extreme Universe Space Observatory, on-board the Japanese Experiment Module of the International Space Station.
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