Model for bubble nucleation efficiency of low-energy nuclear recoils in bubble chambers for dark matter detection
arXiv:2401.15531 · doi:10.1103/PhysRevD.110.022005
Abstract
Bubble chambers are promising technologies for detecting low-energy nuclear recoils from the elastic scattering of dark matter particle candidates. Bubble nucleation occurs when the energy deposition exceeds a specific threshold defined traditionally by the "heat-spike" Seitz threshold. In this paper, we report on a physical model that can account for observed discrepancies between the current Seitz model and the measured nucleation efficiency of low-energy nuclear recoils, which is necessary for interpreting dark matter signals. In our work, we combine molecular dynamics and Monte Carlo simulations together with the Lindhard model to predict bubble nucleation efficiency and energy thresholds for CF, CFI, and xenon with enhanced accuracy over the Seitz model when compared to existing experimental data. We use our model to determine the effect on cross-section limits for spin-dependent and spin-independent interactions and compare it to the current PICO dark matter experiment. Our technique can also be applied to estimate the efficiency of future target fluids where no experimental data are available. As an example, we predict the nucleation efficiency, the energy threshold and the cross-section limits in the spin-independent channel for the Scintillating Bubble Chamber experiment filled with superheated liquid argon.
arXiv comment14 pages
References in corpus (20)
- A Unified Approach to the Classical Statistical Analysis of Small Signals
- Dark Matter Candidates from Particle Physics and Methods of Detection
- First dark matter search results from a 4-kg CFI bubble chamber operated in a deep underground site
- Dark Matter Search Results from the Complete Exposure of the PICO-60 CF Bubble Chamber
- Dark Matter Search Results from the PICO-60 CF Bubble Chamber
- Dark Matter Search Results from the PICO-2L CF Bubble Chamber
- Quantification of Order in the Lennard-Jones System
- Dark Matter Search Results from the PICO-60 CFI Bubble Chamber
- Final Results of the PICASSO Dark Matter Search Experiment
- A Review of Basic Energy Reconstruction Techniques in Liquid Xenon and Argon Detectors for Dark Matter and Neutrino Physics Using NEST
- Identifying the Theory of Dark Matter with Direct Detection
- First Demonstration of a Scintillating Xenon Bubble Chamber for Detecting Dark Matter and Coherent Elastic Neutrino-Nucleus Scattering
- Physics reach of a low threshold scintillating argon bubble chamber in coherent elastic neutrino-nucleus scattering reactor experiments
- Direct Measurement of the Bubble Nucleation Energy Threshold in a CF3I Bubble Chamber
- Bragg-like curve for dark matter searches; binary gases
- Data-Driven Modeling of Electron Recoil Nucleation in PICO CF Bubble Chambers
- Modeling emission of acoustic energy during bubble expansion in PICO bubble chambers
- Determining the bubble nucleation efficiency of low-energy nuclear recoils in superheated CF dark matter detectors
- Molecular dynamics simulations of bubble nucleation in dark matter detectors
- Nucleation efficiency of nuclear recoils in bubble chambers