A parametric approach for the identification of single-charged isotopes with AMS-02

TL;DR

This paper introduces a parametric template fit method leveraging AMS-02 measurements to identify single-charged isotopes in cosmic rays, effectively addressing challenges posed by the dominance of protons over deuterons.

Contribution

The paper presents a novel parametric approach that accounts for systematic uncertainties, improving isotope separation capabilities in AMS-02 data analysis.

Findings

AMS-02 can distinguish hydrogen isotopes up to 10 GeV/n.

The method effectively handles systematic uncertainties and data-simulation differences.

Isotope identification enhances understanding of cosmic ray propagation.

Abstract

Measurements of the isotopic composition of single-charged cosmic rays provide important insights in the propagation processes. However, the isotopic identification is challenging due to the one hundred times greater abundance of protons when compared to deuterons, the only stable isotope of hydrogen. Taking advantage of the precise measurements of the velocity and momentum in the Alpha Magnetic Spectrometer (AMS-02), a particle physics detector operating aboard the International Space Station since May 2011, we describe a parametric template fit method, which takes into account systematic uncertainties such as the fragmentation of particles inside AMS-02 and eventual differences between data and simulation through the use of nuisance parameters. With this method we are also able to assess the AMS-02 performance in terms of mass resolution, showing that it is able to separate the isotopes of hydrogen up to 10 GeV/n.