Antiprotons from Spallations of Cosmic Rays on Interstellar Matter

207 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

A Markov Chain Monte Carlo technique to sample transport and source parameters of Galactic cosmic rays - II. Results for the diffusion model combining B/C and radioactive nuclei (2010, background): “Nevertheless, the results for the 2D geometry are also reported, as it has been used in a series of studies inspecting stable nuclei (Maurin et al. 2001, 2002), β-radioactive nuclei (Donato et al. 2002), standard anti-nuclei (Donato et al. 2001, 2008, 2009) and positrons (Delahaye et al. 2008a).”
Galactic secondary positron flux at the Earth (2008, methodology): “In this analysis, we adopt the determinations of Shikaze et al. (2007) and Donato et al. (2001).”
Sneutrino cold dark matter, a new analysis: Relic abundance and detection rates (2007, methodology): “ statistical experimental uncertainty if the measured antiproton ﬂux consists only in the background (secondary) component. The estimate has been performed by using the background calculation of Ref. [81], and refers to a 1–σstatistical uncertainty. All the supersymmetric conﬁgurations in Fig. 20 ab”
AMS-02 antiprotons, at last! Secondary astrophysical component and immediate implications for Dark Matter (2015, methodology): “Among these, the most relevant ones are the energy distribution in the outcome of inelastic but non-annihilating interactions or elastic scatterings to the extent they do not fully peak in the forward direction, as commonly assumed [55].”