Monte Carlo Simulations of Trapped Ultracold Neutrons in the UCN{\tau} Experiment
Nathan Callahan, Chen-Yu Liu, Francisco Gonzalez, Evan Adamek, James, David Bowman, Leah Broussard, S.M. Clayton, S. Currie, C. Cude-Woods, E.B., Dees, X. Ding, E.M. Egnel, D. Fellers, W. Fox, P. Geltenbort, K.P. Hickerson,, M.A. Hoffbauer, A.T. Holley, A. Komives

TL;DR
This paper presents Monte Carlo simulations of ultracold neutrons in the UCN{ au} experiment, comparing models to experimental data to understand neutron dynamics and improve measurement precision.
Contribution
It introduces a detailed simulation approach for field-trapped ultracold neutrons, highlighting differences from material bottle models and analyzing chaotic dynamics effects.
Findings
Simulation accurately reproduces experimental neutron distributions
Chaotic dynamics influence spectral cleaning and heating effects
Model helps optimize neutron lifetime measurement precision
Abstract
In the UCN{\tau} experiment, ultracold neutrons (UCN) are confined by magnetic fields and the Earth's gravitational field. Field-trapping mitigates the problem of UCN loss on material surfaces, which caused the largest correction in prior neutron experiments using material bottles. However, the neutron dynamics in field traps differ qualitatively from those in material bottles. In the latter case, neutrons bounce off material surfaces with significant diffusivity and the population quickly reaches a static spatial distribution with a density gradient induced by the gravitational potential. In contrast, the field-confined UCN -- whose dynamics can be described by Hamiltonian mechanics -- do not exhibit the stochastic behaviors typical of an ideal gas model as observed in material bottles. In this report, we will describe our efforts to simulate UCN trapping in the UCN{\tau}…
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