1d1b9ef12SLeila Ghaffari // Copyright (c) 2017-2022, Lawrence Livermore National Security, LLC and other CEED contributors. 2d1b9ef12SLeila Ghaffari // All Rights Reserved. See the top-level LICENSE and NOTICE files for details. 3d1b9ef12SLeila Ghaffari // 4d1b9ef12SLeila Ghaffari // SPDX-License-Identifier: BSD-2-Clause 5d1b9ef12SLeila Ghaffari // 6d1b9ef12SLeila Ghaffari // This file is part of CEED: http://github.com/ceed 7d1b9ef12SLeila Ghaffari 8d1b9ef12SLeila Ghaffari /// @file 9d1b9ef12SLeila Ghaffari /// Helper functions for computing stabilization terms of a newtonian simulation 10d1b9ef12SLeila Ghaffari 11d1b9ef12SLeila Ghaffari #ifndef stabilization_h 12d1b9ef12SLeila Ghaffari #define stabilization_h 13d1b9ef12SLeila Ghaffari 14d1b9ef12SLeila Ghaffari #include <ceed.h> 152b916ea7SJeremy L Thompson 16d0cce58aSJeremy L Thompson #include "newtonian_state.h" 17d1b9ef12SLeila Ghaffari 18d1b9ef12SLeila Ghaffari // ***************************************************************************** 1904e40bb6SJeremy L Thompson // Helper function for computing the variation in primitive variables, given Tau_d 20d1b9ef12SLeila Ghaffari // ***************************************************************************** 212b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER void dYFromTau(CeedScalar Y[5], CeedScalar Tau_d[3], CeedScalar dY[5]) { 22d1b9ef12SLeila Ghaffari dY[0] = Tau_d[0] * Y[0]; 23d1b9ef12SLeila Ghaffari dY[1] = Tau_d[1] * Y[1]; 24d1b9ef12SLeila Ghaffari dY[2] = Tau_d[1] * Y[2]; 25d1b9ef12SLeila Ghaffari dY[3] = Tau_d[1] * Y[3]; 26d1b9ef12SLeila Ghaffari dY[4] = Tau_d[2] * Y[4]; 27d1b9ef12SLeila Ghaffari } 28d1b9ef12SLeila Ghaffari 29d1b9ef12SLeila Ghaffari // ***************************************************************************** 30d1b9ef12SLeila Ghaffari // Helper functions for computing the stabilization terms 31d1b9ef12SLeila Ghaffari // ***************************************************************************** 32*51d861cbSJames Wright CEED_QFUNCTION_HELPER void StabilizationMatrix(NewtonianIdealGasContext gas, State s, CeedScalar Tau_d[3], CeedScalar strong_residual[5], 33*51d861cbSJames Wright CeedScalar stab[5][3]) { 34d1b9ef12SLeila Ghaffari CeedScalar dY[5]; 35d1b9ef12SLeila Ghaffari StateConservative dF[3]; 36d1b9ef12SLeila Ghaffari // Zero stab so all future terms can safely sum into it 372b916ea7SJeremy L Thompson for (CeedInt i = 0; i < 5; i++) { 382b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 3; j++) stab[i][j] = 0; 392b916ea7SJeremy L Thompson } 40*51d861cbSJames Wright dYFromTau(strong_residual, Tau_d, dY); 41edcfef1bSKenneth E. Jansen State ds = StateFromY_fwd(gas, s, dY); 42d1b9ef12SLeila Ghaffari FluxInviscid_fwd(gas, s, ds, dF); 43d1b9ef12SLeila Ghaffari for (CeedInt i = 0; i < 3; i++) { 44d1b9ef12SLeila Ghaffari CeedScalar dF_i[5]; 45d1b9ef12SLeila Ghaffari UnpackState_U(dF[i], dF_i); 462b916ea7SJeremy L Thompson for (CeedInt j = 0; j < 5; j++) stab[j][i] += dF_i[j]; 47d1b9ef12SLeila Ghaffari } 48d1b9ef12SLeila Ghaffari } 49d1b9ef12SLeila Ghaffari 502b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER void Stabilization(NewtonianIdealGasContext gas, State s, CeedScalar Tau_d[3], State ds[3], CeedScalar U_dot[5], 51edcfef1bSKenneth E. Jansen const CeedScalar body_force[5], CeedScalar stab[5][3]) { 52d1b9ef12SLeila Ghaffari // -- Stabilization method: none (Galerkin), SU, or SUPG 53*51d861cbSJames Wright CeedScalar strong_residual[5] = {0}; 54d1b9ef12SLeila Ghaffari switch (gas->stabilization) { 55d1b9ef12SLeila Ghaffari case STAB_NONE: 56d1b9ef12SLeila Ghaffari break; 57d1b9ef12SLeila Ghaffari case STAB_SU: 58*51d861cbSJames Wright FluxInviscidStrong(gas, s, ds, strong_residual); 59d1b9ef12SLeila Ghaffari break; 60d1b9ef12SLeila Ghaffari case STAB_SUPG: 61*51d861cbSJames Wright FluxInviscidStrong(gas, s, ds, strong_residual); 62*51d861cbSJames Wright for (CeedInt j = 0; j < 5; j++) strong_residual[j] += U_dot[j] - body_force[j]; 63d1b9ef12SLeila Ghaffari break; 64d1b9ef12SLeila Ghaffari } 65*51d861cbSJames Wright StabilizationMatrix(gas, s, Tau_d, strong_residual, stab); 66d1b9ef12SLeila Ghaffari } 67d1b9ef12SLeila Ghaffari 68d1b9ef12SLeila Ghaffari // ***************************************************************************** 69d1b9ef12SLeila Ghaffari // Helper function for computing Tau elements (stabilization constant) 70d1b9ef12SLeila Ghaffari // Model from: 71d1b9ef12SLeila Ghaffari // PHASTA 72d1b9ef12SLeila Ghaffari // 73d1b9ef12SLeila Ghaffari // Tau[i] = itau=0 which is diagonal-Shakib (3 values still but not spatial) 74d1b9ef12SLeila Ghaffari // ***************************************************************************** 752b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER void Tau_diagPrim(NewtonianIdealGasContext gas, State s, const CeedScalar dXdx[3][3], const CeedScalar dt, 762b916ea7SJeremy L Thompson CeedScalar Tau_d[3]) { 77d1b9ef12SLeila Ghaffari // Context 78d1b9ef12SLeila Ghaffari const CeedScalar Ctau_t = gas->Ctau_t; 79d1b9ef12SLeila Ghaffari const CeedScalar Ctau_v = gas->Ctau_v; 80d1b9ef12SLeila Ghaffari const CeedScalar Ctau_C = gas->Ctau_C; 81d1b9ef12SLeila Ghaffari const CeedScalar Ctau_M = gas->Ctau_M; 82d1b9ef12SLeila Ghaffari const CeedScalar Ctau_E = gas->Ctau_E; 83d1b9ef12SLeila Ghaffari const CeedScalar cv = gas->cv; 84d1b9ef12SLeila Ghaffari const CeedScalar mu = gas->mu; 85d1b9ef12SLeila Ghaffari const CeedScalar rho = s.U.density; 86d1b9ef12SLeila Ghaffari 87d1b9ef12SLeila Ghaffari CeedScalar tau; 88d1b9ef12SLeila Ghaffari CeedScalar dts; 89d1b9ef12SLeila Ghaffari CeedScalar fact; 90d1b9ef12SLeila Ghaffari 91d5eb0e14SJames Wright CeedScalar gijd_mat[3][3] = {{0.}}, velocity_term; 92d5eb0e14SJames Wright MatMat3(dXdx, dXdx, CEED_TRANSPOSE, CEED_NOTRANSPOSE, gijd_mat); 93d1b9ef12SLeila Ghaffari 94d1b9ef12SLeila Ghaffari dts = Ctau_t / dt; 95d1b9ef12SLeila Ghaffari 96d5eb0e14SJames Wright { // u_i g_ij u_j 97d5eb0e14SJames Wright CeedScalar gij_uj[3] = {0.}; 98d5eb0e14SJames Wright MatVec3(gijd_mat, s.Y.velocity, CEED_NOTRANSPOSE, gij_uj); 99d5eb0e14SJames Wright velocity_term = Dot3(s.Y.velocity, gij_uj); 100d5eb0e14SJames Wright } 101d5eb0e14SJames Wright 102d5eb0e14SJames Wright tau = Square(rho) * (4. * Square(dts) + velocity_term) + Ctau_v * Square(mu) * DotN((CeedScalar *)gijd_mat, (CeedScalar *)gijd_mat, 9); 103d1b9ef12SLeila Ghaffari 104d1b9ef12SLeila Ghaffari fact = sqrt(tau); 105d1b9ef12SLeila Ghaffari 106d5eb0e14SJames Wright Tau_d[0] = Ctau_C * fact / (rho * (gijd_mat[0][0] + gijd_mat[1][1] + gijd_mat[2][2])) * 0.125; 107d1b9ef12SLeila Ghaffari Tau_d[1] = Ctau_M / fact; 108d1b9ef12SLeila Ghaffari Tau_d[2] = Ctau_E / (fact * cv); 109d1b9ef12SLeila Ghaffari 11004e40bb6SJeremy L Thompson // consider putting back the way I initially had it 11104e40bb6SJeremy L Thompson // Ctau_E * Tau_d[1] /cv to avoid a division if the compiler is smart enough to see that cv IS a constant that it could invert once for all elements 112d1b9ef12SLeila Ghaffari // but in that case energy tau is scaled by the product of Ctau_E * Ctau_M 11304e40bb6SJeremy L Thompson // OR we could absorb cv into Ctau_E but this puts more burden on user to know how to change constants with a change of fluid or units. Same for 114d1b9ef12SLeila Ghaffari // Ctau_v * mu * mu IF AND ONLY IF we don't add viscosity law =f(T) 115d1b9ef12SLeila Ghaffari } 116d1b9ef12SLeila Ghaffari 117d1b9ef12SLeila Ghaffari // ***************************************************************************** 118d1b9ef12SLeila Ghaffari 119d1b9ef12SLeila Ghaffari #endif // stabilization_h 120