Fresh Insights on Cosmic-ray Propagation from the New AMS Data
Nicola Tomassetti, Jie Feng, Alberto Oliva
TL;DR
This paper analyzes new AMS cosmic-ray data at TeV energies using a Bayesian approach to refine models of cosmic-ray propagation in the galaxy.
Contribution
It introduces a global Bayesian analysis of cosmic-ray transport models based on recent AMS measurements, providing fresh insights into cosmic-ray propagation.
Findings
Refined parameters for cosmic-ray transport models
Enhanced understanding of primary and secondary nuclei ratios
Constraints on cosmic-ray diffusion coefficients
Abstract
The Alpha Magnetic Spectrometer (AMS) experiment has released new measurements of primary and secondary nuclei in cosmic rays at the TeV energy scale. Using these data, we present new results based on a global Bayesian analysis of our two halo model of CR transport.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.