pub const SE_BSE_SPLIT_EV: f64 = 50.0;Expand description
Default SE/BSE energy split, eV: an escaping electron below this energy is
in the secondary (slow) class, at or above it in the backscattered (fast)
class. Chen et al., Sci. Rep. 12, 18201 (2022),
doi:10.1038/s41598-022-20466-3, Introduction and section “Monte Carlo
simulation”; the assignment of the boundary itself follows Nebula’s
DETECTOR_GE50 flag. See the module docs.