Developing Algorithms for Bubble Identification and Tracking for the PICO-40L Dark Matter Experiment

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Authors

Bai, Minya

Date

2025-05-02

Type

thesis

Language

eng

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WIMPs , Dark matter , Bubble chamber , Particle physics , Optics analysis , Bubble motion

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Abstract

The understanding of cosmological dark matter is one of the major challenges in modern physics. Weakly interacting massive particles (WIMPs) are a popular candidate for dark matter that have been probed by detectors attempting to measure nuclear recoils from WIMP interactions. The PICO experiment aims to use bubble chambers to search for spin-dependent WIMP-proton dark matter. Acoustic data and optical images of the bubbles are used to identify the particle interacting with the fluid in the detector. WIMP interactions with the active fluid will result in a single bubble event that is acoustically similar to a neutron. Higher resolution between single and multi-bubble events can provide a secondary method to confirm the multiplicity of neutron events. The Watershed algorithm was developed as a viable option to better resolve bubbles that formed closed together. PICO-40L is a prototype detector that is being used to test the engineering design that will be used in the next generation PICO-500 detector. The motion of the bubbles was studied to determine the effects of convection within the active fluid. The position reconstruction agreed well with to the calculated terminal velocity of the bubbles. An asymmetry in the vertical velocity was observed within the bulk of the detector indicating the presence of convection within the active volume, which might be related to spurious background events that have been observed in PICO-40L.

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