Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays: Results from AMS-01
Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propag...
Similar Items
-
ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01
by: Becker, R., et al.
Published: (2014) -
Generalized event shape and energy flow studies in e[superscript +]e[superscript −] annihilation at √s = 91.2−208.0 GeV
by: Berges, P., et al.
Published: (2015) -
Test of the tau-model of Bose-Einstein correlations and reconstruction of the source function in hadronic Z-boson decay at LEP
by: Becker, Ulrich J., et al.
Published: (2013) -
Electroweak measurements in electron–positron collisions at W-boson-pair energies at LEP
by: Becker, Ulrich J, et al.
Published: (2019) -
First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV
by: Basil, A., et al.
Published: (2013)