PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energy.
Adriani O, Barbarino GC, Bazilevskaya GA, Bellotti R, Boezio M, Bogomolov EA, Bonechi L, Bongi M, Bonvicini V, Borisov S, Bottai S, Bruno A, Cafagna F, Campana D, Carbone R, Carlson P, Casolino M, Castellini G, Consiglio L, De Pascale MP, De Santis C, De Simone N, Di Felice V, Galper AM, Gillard W, Grishantseva L, Hofverberg P, Jerse G, Karelin AV, Koldashov SV, Krutkov SY, Kvashnin AN, Leonov A, Malvezzi V, Marcelli L, Mayorov AG, Menn W, Mikhailov VV, Mocchiutti E, Monaco A, Mori N, Nikonov N, Osteria G, Papini P, Pearce M, Picozza P, Pizzolotto C, Ricci M, Ricciarini SB, Rossetto L, Simon M, Sparvoli R, Spillantini P, Stozhkov YI, Vacchi A, Vannuccini E, Vasilyev G, Voronov SA, Wu J, Yurkin YT, Zampa G, Zampa N, Zverev VG.
Adriani O, et al. Among authors: hofverberg p.
Phys Rev Lett. 2010 Sep 17;105(12):121101. doi: 10.1103/PhysRevLett.105.121101. Epub 2010 Sep 13.
Phys Rev Lett. 2010.
PMID: 20867623