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On nuclear coalescence in small interacting systems
M. Kachelriess, S. Ostapchenko, J. Tjemsland
The formation of light nuclei can be described as the coalescence of clusters of nucleons into nuclei. In the case of small interacting systems, such as dark matter and an…
Self-consistent approach for measuring the energy spectra and composition of cosmic rays and determining the properties of hadronic interactions at high energy
Andrea Addazi, Andy Buckley, Jose Bellido +25
Air showers, produced by the interaction of energetic cosmic rays with the atmosphere, are an excellent alternative to study particle physics at energies beyond any human-made part…
Revisiting cosmic ray antinuclei fluxes with a new coalescence model
M. Kachelriess, S. Ostapchenko, J. Tjemsland
Antideuteron and antihelium nuclei have been proposed as promising detection channels for dark matter because of the low astrophysical backgrounds expected. To estimate both potent…