12b89d87eSLeila Ghaffari // Copyright (c) 2017-2022, Lawrence Livermore National Security, LLC and other CEED contributors. 22b89d87eSLeila Ghaffari // All Rights Reserved. See the top-level LICENSE and NOTICE files for details. 32b89d87eSLeila Ghaffari // 42b89d87eSLeila Ghaffari // SPDX-License-Identifier: BSD-2-Clause 52b89d87eSLeila Ghaffari // 62b89d87eSLeila Ghaffari // This file is part of CEED: http://github.com/ceed 72b89d87eSLeila Ghaffari 82b89d87eSLeila Ghaffari /// @file 92b89d87eSLeila Ghaffari /// Helper functions for computing stabilization terms of a newtonian simulation 102b89d87eSLeila Ghaffari 112b89d87eSLeila Ghaffari #ifndef stabilization_h 122b89d87eSLeila Ghaffari #define stabilization_h 132b89d87eSLeila Ghaffari 142b89d87eSLeila Ghaffari #include <ceed.h> 152b730f8bSJeremy L Thompson 16c9c2c079SJeremy L Thompson #include "newtonian_state.h" 172b89d87eSLeila Ghaffari 182b89d87eSLeila Ghaffari // ***************************************************************************** 19ea61e9acSJeremy L Thompson // Helper function for computing the variation in primitive variables, given Tau_d 202b89d87eSLeila Ghaffari // ***************************************************************************** 212b730f8bSJeremy L Thompson CEED_QFUNCTION_HELPER void dYFromTau(CeedScalar Y[5], CeedScalar Tau_d[3], CeedScalar dY[5]) { 222b89d87eSLeila Ghaffari dY[0] = Tau_d[0] * Y[0]; 232b89d87eSLeila Ghaffari dY[1] = Tau_d[1] * Y[1]; 242b89d87eSLeila Ghaffari dY[2] = Tau_d[1] * Y[2]; 252b89d87eSLeila Ghaffari dY[3] = Tau_d[1] * Y[3]; 262b89d87eSLeila Ghaffari dY[4] = Tau_d[2] * Y[4]; 272b89d87eSLeila Ghaffari } 282b89d87eSLeila Ghaffari 292b89d87eSLeila Ghaffari // ***************************************************************************** 302b89d87eSLeila Ghaffari // Helper functions for computing the stabilization terms 312b89d87eSLeila Ghaffari // ***************************************************************************** 32a600bde5SKenneth E. Jansen CEED_QFUNCTION_HELPER void StabilizationMatrix(NewtonianIdealGasContext gas, State s, CeedScalar Tau_d[3], CeedScalar R[5], CeedScalar stab[5][3]) { 332b89d87eSLeila Ghaffari CeedScalar dY[5]; 342b89d87eSLeila Ghaffari StateConservative dF[3]; 352b89d87eSLeila Ghaffari // Zero stab so all future terms can safely sum into it 362b730f8bSJeremy L Thompson for (CeedInt i = 0; i < 5; i++) { 372b730f8bSJeremy L Thompson for (CeedInt j = 0; j < 3; j++) stab[i][j] = 0; 382b730f8bSJeremy L Thompson } 392b89d87eSLeila Ghaffari dYFromTau(R, Tau_d, dY); 403bd61617SKenneth E. Jansen State ds = StateFromY_fwd(gas, s, dY); 412b89d87eSLeila Ghaffari FluxInviscid_fwd(gas, s, ds, dF); 422b89d87eSLeila Ghaffari for (CeedInt i = 0; i < 3; i++) { 432b89d87eSLeila Ghaffari CeedScalar dF_i[5]; 442b89d87eSLeila Ghaffari UnpackState_U(dF[i], dF_i); 452b730f8bSJeremy L Thompson for (CeedInt j = 0; j < 5; j++) stab[j][i] += dF_i[j]; 462b89d87eSLeila Ghaffari } 472b89d87eSLeila Ghaffari } 482b89d87eSLeila Ghaffari 492b730f8bSJeremy L Thompson CEED_QFUNCTION_HELPER void Stabilization(NewtonianIdealGasContext gas, State s, CeedScalar Tau_d[3], State ds[3], CeedScalar U_dot[5], 503bd61617SKenneth E. Jansen const CeedScalar body_force[5], CeedScalar stab[5][3]) { 512b89d87eSLeila Ghaffari // -- Stabilization method: none (Galerkin), SU, or SUPG 522b89d87eSLeila Ghaffari CeedScalar R[5] = {0}; 532b89d87eSLeila Ghaffari switch (gas->stabilization) { 542b89d87eSLeila Ghaffari case STAB_NONE: 552b89d87eSLeila Ghaffari break; 562b89d87eSLeila Ghaffari case STAB_SU: 572b89d87eSLeila Ghaffari FluxInviscidStrong(gas, s, ds, R); 582b89d87eSLeila Ghaffari break; 592b89d87eSLeila Ghaffari case STAB_SUPG: 602b89d87eSLeila Ghaffari FluxInviscidStrong(gas, s, ds, R); 612b89d87eSLeila Ghaffari for (CeedInt j = 0; j < 5; j++) R[j] += U_dot[j] - body_force[j]; 622b89d87eSLeila Ghaffari break; 632b89d87eSLeila Ghaffari } 643bd61617SKenneth E. Jansen StabilizationMatrix(gas, s, Tau_d, R, stab); 652b89d87eSLeila Ghaffari } 662b89d87eSLeila Ghaffari 672b89d87eSLeila Ghaffari // ***************************************************************************** 682b89d87eSLeila Ghaffari // Helper function for computing Tau elements (stabilization constant) 692b89d87eSLeila Ghaffari // Model from: 702b89d87eSLeila Ghaffari // PHASTA 712b89d87eSLeila Ghaffari // 722b89d87eSLeila Ghaffari // Tau[i] = itau=0 which is diagonal-Shakib (3 values still but not spatial) 732b89d87eSLeila Ghaffari // ***************************************************************************** 742b730f8bSJeremy L Thompson CEED_QFUNCTION_HELPER void Tau_diagPrim(NewtonianIdealGasContext gas, State s, const CeedScalar dXdx[3][3], const CeedScalar dt, 752b730f8bSJeremy L Thompson CeedScalar Tau_d[3]) { 762b89d87eSLeila Ghaffari // Context 772b89d87eSLeila Ghaffari const CeedScalar Ctau_t = gas->Ctau_t; 782b89d87eSLeila Ghaffari const CeedScalar Ctau_v = gas->Ctau_v; 792b89d87eSLeila Ghaffari const CeedScalar Ctau_C = gas->Ctau_C; 802b89d87eSLeila Ghaffari const CeedScalar Ctau_M = gas->Ctau_M; 812b89d87eSLeila Ghaffari const CeedScalar Ctau_E = gas->Ctau_E; 822b89d87eSLeila Ghaffari const CeedScalar cv = gas->cv; 832b89d87eSLeila Ghaffari const CeedScalar mu = gas->mu; 842b89d87eSLeila Ghaffari const CeedScalar rho = s.U.density; 852b89d87eSLeila Ghaffari 862b89d87eSLeila Ghaffari CeedScalar tau; 872b89d87eSLeila Ghaffari CeedScalar dts; 882b89d87eSLeila Ghaffari CeedScalar fact; 892b89d87eSLeila Ghaffari 90*b9b033b3SJames Wright CeedScalar gijd_mat[3][3] = {{0.}}, velocity_term; 91*b9b033b3SJames Wright MatMat3(dXdx, dXdx, CEED_TRANSPOSE, CEED_NOTRANSPOSE, gijd_mat); 922b89d87eSLeila Ghaffari 932b89d87eSLeila Ghaffari dts = Ctau_t / dt; 942b89d87eSLeila Ghaffari 95*b9b033b3SJames Wright { // u_i g_ij u_j 96*b9b033b3SJames Wright CeedScalar gij_uj[3] = {0.}; 97*b9b033b3SJames Wright MatVec3(gijd_mat, s.Y.velocity, CEED_NOTRANSPOSE, gij_uj); 98*b9b033b3SJames Wright velocity_term = Dot3(s.Y.velocity, gij_uj); 99*b9b033b3SJames Wright } 100*b9b033b3SJames Wright 101*b9b033b3SJames Wright tau = Square(rho) * (4. * Square(dts) + velocity_term) + Ctau_v * Square(mu) * DotN((CeedScalar *)gijd_mat, (CeedScalar *)gijd_mat, 9); 1022b89d87eSLeila Ghaffari 1032b89d87eSLeila Ghaffari fact = sqrt(tau); 1042b89d87eSLeila Ghaffari 105*b9b033b3SJames Wright Tau_d[0] = Ctau_C * fact / (rho * (gijd_mat[0][0] + gijd_mat[1][1] + gijd_mat[2][2])) * 0.125; 1062b89d87eSLeila Ghaffari Tau_d[1] = Ctau_M / fact; 1072b89d87eSLeila Ghaffari Tau_d[2] = Ctau_E / (fact * cv); 1082b89d87eSLeila Ghaffari 109ea61e9acSJeremy L Thompson // consider putting back the way I initially had it 110ea61e9acSJeremy 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 1112b89d87eSLeila Ghaffari // but in that case energy tau is scaled by the product of Ctau_E * Ctau_M 112ea61e9acSJeremy 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 1132b89d87eSLeila Ghaffari // Ctau_v * mu * mu IF AND ONLY IF we don't add viscosity law =f(T) 1142b89d87eSLeila Ghaffari } 1152b89d87eSLeila Ghaffari 1162b89d87eSLeila Ghaffari // ***************************************************************************** 1172b89d87eSLeila Ghaffari 1182b89d87eSLeila Ghaffari #endif // stabilization_h 119