Sharp Increasing of Positron to Electron Fluxes Ratio below 2 GV Measured by the PAMELA
V. V. Mikhailov,O. Adriani,G. Barbarino,G. A. Bazilevskaya,R. Bellotti,M. Boezio,E. A. Bogomolov,M. Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. S. Cafagna,D. Campana,P. Carlson,M. Casolino,G. Castellini,C. De Donato,C. De Santis,N. De Simone,V. Di Felice,A. M. Galper,A. V. Karelin,S. V. Koldashov, S. Koldobsky,S. Yu Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,L. Marcelli,M. Martucci,A. G. Mayorov,W. Menn,M. Merge,E. Mocchiutti,A. Monaco,N. Mori,R. Munini,G. Osteria,P. Papini,F. Palma,B. Panico,M. Pearce,P. Picozza,M. Ricci,S. B. Ricciarini,M. Simon,R. Sparvoli,P. Spillantini,Yu I. Stozhkov,A. Vacchi,E. Vannuccini,G. I. Vasiliev,S. A. Voronov,Yu T. Yurkin,G. Zampa,N. Zampa INTERNATIONAL CONFERENCE ON PARTICLE PHYSICS AND ASTROPHYSICS(2017)
AI Read Science
Must-Reading Tree
Example

Generate MRT to find the research sequence of this paper