Scintillating Bubble Chamber collaboration is searching for weakly interacting massive particles using a novel bubble chamber with intended thresholds as low as 100 eV. Existing molecular dynamics simulations of bubble formation in bubble chambers were conducted with nonscintillating target materials and therefore do not account for the energy transfer to photons or time-delayed releases that occur in atomic de-excitation. In this study, we use the HOOMD-blue molecular dynamics framework to simulate bubble formation in liquid argon, including photon creation, ionization, and direct nuclear recoils. A multistage bubble growth process similar to that reported in the literature was observed. When comparing simulated thresholds with and without scintillation effects, we found that scintillation raises the average energy required to form a bubble by a factor of 2.16. This is larger than the fraction of energy lost to photon creation and demonstrates that energy stored in excited molecular states with lifetimes longer than the rapid growth phase of nucleation ($\sim 250\mathrm{ps}$) does not contribute significantly to bubble formation. This conclusion was further supported by simulations showing increased bubble nucleation thresholds when the excited molecular state lifetimes were increased, even under identical thermodynamic conditions.

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• Bubble dynamics
• Dark matter
• Molecular dynamics
• Monte Carlo methods