Merge branch 'chongchong/kappa-int-v8.2' of https://github.com/quokka…

…-astro/quokka into chongchong/kappa-int-v8.2
quokka-astro · May 6, 2024 · 1aa1d6a · 1aa1d6a
2 parents 2dc7431 + 7fd5d63
commit 1aa1d6a
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Showing 2 changed files with 7 additions and 5 deletions.
diff --git a/src/RadhydroPulseMGint/test_radhydro_pulse_MG_int.cpp b/src/RadhydroPulseMGint/test_radhydro_pulse_MG_int.cpp
@@ -12,7 +12,7 @@
 #include "radiation_system.hpp"
 
 struct MGProblem {
-};		     // dummy type to allow compile-type polymorphism via template specialization
+}; // dummy type to allow compile-type polymorphism via template specialization
 struct ExactProblem {
 };
 
@@ -125,7 +125,7 @@ template <> struct RadSystem_Traits<ExactProblem> {
 template <>
 template <typename ArrayType>
 AMREX_GPU_HOST_DEVICE auto RadSystem<MGProblem>::ComputeRadQuantityExponents(ArrayType const & /*quant*/,
-										amrex::GpuArray<double, nGroups_ + 1> const & /*boundaries*/)
+									     amrex::GpuArray<double, nGroups_ + 1> const & /*boundaries*/)
     -> amrex::GpuArray<double, nGroups_>
 {
 	amrex::GpuArray<double, nGroups_> exponents{};
@@ -186,7 +186,8 @@ template <> AMREX_GPU_HOST_DEVICE auto RadSystem<ExactProblem>::ComputePlanckOpa
 	return kappaPVec;
 }
 
-template <> AMREX_GPU_HOST_DEVICE auto RadSystem<ExactProblem>::ComputeFluxMeanOpacity(const double rho, const double Tgas) -> quokka::valarray<double, nGroups_>
+template <>
+AMREX_GPU_HOST_DEVICE auto RadSystem<ExactProblem>::ComputeFluxMeanOpacity(const double rho, const double Tgas) -> quokka::valarray<double, nGroups_>
 {
 	const double sigma = 101.248 * std::pow(Tgas / T0, -3.5);
 	quokka::valarray<double, nGroups_> kappaPVec{};

diff --git a/src/radiation_system.hpp b/src/radiation_system.hpp
@@ -53,8 +53,9 @@ static const bool use_wavespeed_correction = false;
 
 // enum for opacity_model
 enum OpacityModel {
-	user = 0, // user-defined opacity for each group, given as a function of density and temperature.
-	piecewisePowerLaw // piecewise power-law opacity model with piecewise power-law fitting to a user-defined opacity function and on-the-fly piecewise power-law fitting to radiation energy density and flux.
+	user = 0,	  // user-defined opacity for each group, given as a function of density and temperature.
+	piecewisePowerLaw // piecewise power-law opacity model with piecewise power-law fitting to a user-defined opacity function and on-the-fly piecewise
+			  // power-law fitting to radiation energy density and flux.
 };
 
 // this struct is specialized by the user application code