Right now it's hard coded to assume all sampled particles are born at t = 0. This is probably appropriate for most scenarios but doesn't feel like a satisfactory solution. This could be addressed with a delta function (similar to how mono-energetic distributions are being handled).
If time distributions are added, we need to be careful about how this would interact with any future temporal functionality. If a particle is born into a time that doesn't correspond to the "time" of the plasma state currently being simulated, we'd have to be able to address that.
Right now it's hard coded to assume all sampled particles are born at t = 0. This is probably appropriate for most scenarios but doesn't feel like a satisfactory solution. This could be addressed with a delta function (similar to how mono-energetic distributions are being handled).
If time distributions are added, we need to be careful about how this would interact with any future temporal functionality. If a particle is born into a time that doesn't correspond to the "time" of the plasma state currently being simulated, we'd have to be able to address that.