A comprehensive simulation of the thermal noise background observed in UHE radio-frequency neutrino detectors. Includes a parallelized "inverse" Monte Carlo radiation transport code (allowing for the modeling of birefringent and highly anisotropic media), a precise model of the Johnson-Nyquist contribution (including quantum effects), and a Markov Chain model of the simple multiplicity and phased array triggers.
The complete parallelized Monte Carlo radiation transport code relies heavily on details of the specific hardware on which it was intended to be run, and a decoupled version has not yet been uploaded.