Higgs Portal From The Atmosphere To Hyper-K
Paul Archer-Smith, Yue Zhang

TL;DR
This paper proposes using the Hyper-Kamiokande detector to search for light Higgs portal scalars produced in the atmosphere, which decay into electron-positron pairs, offering a new way to explore uncharted particle physics parameter space.
Contribution
It introduces a novel atmospheric production and detection method for Higgs portal scalars using large neutrino detectors, expanding the search beyond traditional beam experiments.
Findings
Hyper-Kamiokande can probe new parameter space for light scalars.
Atmospheric production of scalars leads to detectable electron-positron pairs.
The method is complementary to existing intensity frontier experiments.
Abstract
A light Higgs portal scalar could be abundantly produced in the earth's atmosphere and decay in large-volume neutrino detectors. We point out that the Hyper-Kamiokande detector bears a strong discovery potential of probing such particles in an uncharted parameter space that is actively explored by intensity frontier experiments including rare kaon decays. The signal we propose to look for is electron-positron pair creation that manifests as a double-ring appearing from the same vertex. Most of these pairs originate from zenith angles above the Hyper-K detector's horizon. This search can be generalized to other new light states and is highly complementary to beam experiments.
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.
