Closed srichers closed 3 years ago
Cool! Do you have a reference for these closure parameters?
Minerbo 1978 https://www.sciencedirect.com/science/article/abs/pii/0022407378900249 I'll add it to a comment
The Fiducial runs set up the initial distribution as linear in costheta (where theta is the angle between the neutrino direction and the flux direction). But most moment-based radiation transport simulations assume the distribution is exponential with costheta. So this sets up a new type of problem that follows the same assumptions as those used in the transport calculations. This will allow us to, say, grab a position in a 3D simulation of a neutron star merger and simulate those parameters.
Add in initial condition method that allows us to input the density and flux vector of each species.