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Modeling emission of acoustic energy during bubble expansion in PICO bubble chambers

Tetiana Kozynets*, Scott Fallows, and Carsten B. Krauss

  • Department of Physics, University of Alberta, Edmonton T6G 2E1, Canada

  • *kozynets@ualberta.ca

Phys. Rev. D 100, 052001 – Published 3 September, 2019

DOI: https://doi.org/10.1103/PhysRevD.100.052001

Abstract

The PICO experiment uses bubble chambers filled with superheated C3F8 for spin-dependent weakly interacting massive particle (WIMP) dark matter searches. One of the main sources of background in these detectors is alpha particles from decays of environmental Rn222, which nucleate bubbles that are visually indistinguishable from WIMP candidate events. Alpha-induced bubbles can be discriminated acoustically, because the signal from alpha events is consistently larger in magnitude than that from nuclear-recoil-/WIMP-like events. By studying the dynamics of bubbles nucleated by these two types of ionizing radiation from the first stages of their growth, we present a physical model for the acoustic discrimination for the first time. The distribution of acoustic energies that we generate for a simulated sample of bubble nucleations by alpha particles and nuclear recoils is compared directly to the experimental data.

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