Formation of light (anti)nuclei

TL;DR

This paper introduces a new coalescence model for light (anti)nuclei production, incorporating process-dependent formation region size and momentum correlations, validated against experimental data across various collision types.

Contribution

The paper presents a novel coalescence model that accounts for formation region size and momentum correlations, improving predictions of light (anti)nuclei yields in high-energy collisions.

Findings

Model agrees well with experimental data on antideuteron and antihelium-3 production.

Incorporates process-dependent formation region size and momentum correlations.

Validated across multiple collision types and energies.

Abstract

The production mechanism of light nuclei, such as deuteron, helium-3, tritium and their antiparticles, has recently attracted an increased attention from the astroparticle and heavy ion communities. The expected low astrophysical background of light antinulei makes them ideal probes for exotic astrophysical processes, such as dark matter annihilations. At the same time, they can be used to measure two-nucleon correlations and density fluctuations in heavy ion collisions, which may shed light on the QCD phase diagram. Motivated by the importance of light antinuclei in cosmic ray studies, we developed a new coalescence model for light (anti)nuclei that includes both the size of the formation region, which is process dependent, and momentum correlations in a semi-classical picture. We have employed the model as an afterburner to the event generators Pythia 8 and QGSJET II, and find that the model agrees well with experimental data on antideuteron and antihelium-3 production in $e^+e^-$, $pp$, $p$Be and $p$Al collisions at various energies. In this paper, we review this model and update existing fits to experimental data based on new insights.