Cosmic Rays below Z = 30 in a Diffusion Model: New Constraints on Propagation Parameters

By D. Maurin, F. Donato, R. Taillet, P. Salati. 2001

346 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/987afc69cf57733c7a131bd9c3a2f5b6da5caac3

How researchers see this paper

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

In Astronomy and Astrophysics

1. N. Fornengo
2. R. Lineros
3. A. Putze
4. L. Derome
5. D. Maurin
6. D. Maurin
7. R. Taillet
8. P. Ullio

In Nuclear and High Energy Physics

1. N. Fornengo
2. R. Lineros
3. J. Lavalle
4. T. Delahaye
5. L. Derome
6. A. Putze
7. D. Maurin
8. P. Salati

Citations in the corpus

• Galactic secondary positron flux at the Earth (2008, methodology): “Third, the uncertainties in the propagation parameters involved in the diffusion equation were thoroughly studied (Maurin et al. 2001).”
• A database of charged cosmic rays (2013, methodology): “The CR data are the backbone of Galactic CR propagation studies (e.g., Jones et al. 2001; Maurin et al. 2001; Strong et al. 2007; Evoli et al. 2008).”
• Cosmic-ray propagation with DRAGON2: I. numerical solver and astrophysical ingredients (2016, methodology): “3 Semi-analytical solutions of the propagation equation are implemented in the USINE code developed since 2010 [41].”
• Antiprotons from Spallations of Cosmic Rays on Interstellar Matter (2001, methodology): “We propose to go beyond this type of study and to use the results of our systematic analysis of nuclei (Maurin et al. 2001, hereafter Paper I) to ascertain the theoretical uncertainties on the interstellar secondary antiproton energy spectrum.”
• 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, methodology): “Several diffusion models are considered in the literature (Webber et al. 1992; Bloemen et al. 1993; Strong & Moskalenko 1998; Jones et al. 2001; Maurin et al. 2001; Berezhko et al. 2003; Shibata et al. 2006; Evoli et al. 2008; Farahat et al. 2008).”
• Interpretation of AMS-02 electrons and positrons data (2014, background): “[171] and compatible with the boron-tocarbon analysis [170].”
• Dark matter annihilations and decays after the AMS-02 positron measurements (2013, background): “Information on the parameters K0, δ and L can be inferred from the flux measurements of other cosmic ray species, mainly from the boron-to-carbon ratio [30].”