2013/04/03 by M. Aguilar, G. Alberti, B. Alpat +97 · 1,062 citations
Physics and Astronomy · #Anisotropy #Antimatter #Astrophysics and Cosmic Phenomena #Atomic physics #Cosmic ray #Dark Matter and Cosmic Phenomena #Electron #International Space Station #Materials science #Nuclear physics #Observable #Optics #PAMELA detector #Particle physics theoretical and experimental studies #Physics #Positron #Range (aeronautics) #Spectrometer #Ultra-high-energy cosmic ray
paper · pdf · doi:10.1103/physrevlett.110.141102
published in Physical Review Letters 110(14), 141102 (American Physical Society)
openalex publication_date 2013/04/03 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
A precision measurement by the Alpha Magnetic Spectrometer on the International Space Station of the positron fraction in primary cosmic rays in the energy range from 0.5 to 350 GeV based on 6.8 × 10(6) positron and electron events is presented. The very accurate data show that the positron fraction is steadily increasing from 10 to ∼ 250 GeV, but, from 20 to 250 GeV, the slope decreases by an order of magnitude. The positron fraction spectrum shows no fine structure, and the positron to electron ratio shows no observable anisotropy. Together, these features show the existence of new physical phenomena.