Where do the AMS-02 anti-helium events come from?
Vivian Poulin, Pierre Salati, Ilias Cholis, Marc Kamionkowski, and, Joseph Silk

TL;DR
This paper investigates the possible origins of anti-helium events detected by AMS-02, concluding that conventional spallation and dark matter explanations are unlikely, and exploring anti-matter regions like anti-clouds or anti-stars as potential sources.
Contribution
It introduces the hypothesis that anti-helium events may originate from anti-matter regions such as anti-clouds or anti-stars, supported by new constraints and observational considerations.
Findings
Spallation predicts anti-helium flux below AMS-02 sensitivity.
Dark matter annihilation unlikely explains the anti-helium events.
Anti-clouds or anti-stars could be the source, with specific properties and constraints.
Abstract
We discuss the origin of the anti-helium-3 and -4 events possibly detected by AMS-02. Using up-to-date semi-analytical tools, we show that spallation from primary hydrogen and helium nuclei onto the ISM predicts a flux typically one to two orders of magnitude below the sensitivity of AMS-02 after 5 years, and a flux roughly 5 orders of magnitude below the AMS-02 sensitivity. We argue that dark matter annihilations face similar difficulties in explaining this event. We then entertain the possibility that these events originate from anti-matter-dominated regions in the form of anti-clouds or anti-stars. In the case of anti-clouds, we show how the isotopic ratio of anti-helium nuclei might suggest that BBN has happened in an inhomogeneous manner, resulting in anti-regions with a anti-baryon-to-photon ratio .…
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.
