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Implement an X-Ray Thomson Scattering (XRTS) module #24
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I think the easiest simulation to get up and running (which still has some depth to it) would be to simulate the free electron component of the XRTS in the random phase approximation (RPA) regime. Scattered spectrum power is related to the dynamic structure factor S(k,w) as well as the incident and scattered wavevectors: Here is the Dynamic Structure Factor equation for the free electron component: Probably the most complicated part of it is doing the complex-valued triple integral for the dielectric function (in the RPA regime), but if it is done in a general enough way, you can use this function with various input distribution functions: We want to use the Fermi-Dirac distribution specifically to describe degenerate electrons in the warm dense matter regime: The chemical potential in the above distribution function can be described by an interpolation between classical and quantum theories, given by: where the coefficients are Note that as temperature T goes large, the above distribution function reduces to the Maxwell-Boltzmann function, so it's still valid for classical plasmas. This interpolated chemical potential is already implemented in PlasmaPy here. |
The integral can be done by splitting into a double integral and a Cauchy integral. For the double integral, I think we can use And since these integrals are being dong at every value of photon energy in the simulation space, we might be able to further optimize this by using |
We already have some optical Thomson Scattering features in PlasmaPy, but it would be good to extend these into the XRTS and warm dense matter regimes, where Compton scattering features, and electron degeneracy, and chemical potentials become important.
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