15aed82e4SJeremy L Thompson // Copyright (c) 2017-2024, 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 10*c0b5abf0SJeremy L Thompson #include <ceed/types.h> 112b730f8bSJeremy L Thompson 12c9c2c079SJeremy L Thompson #include "newtonian_state.h" 132b89d87eSLeila Ghaffari 142b89d87eSLeila Ghaffari // ***************************************************************************** 15ea61e9acSJeremy L Thompson // Helper function for computing the variation in primitive variables, given Tau_d 162b89d87eSLeila Ghaffari // ***************************************************************************** 172b730f8bSJeremy L Thompson CEED_QFUNCTION_HELPER void dYFromTau(CeedScalar Y[5], CeedScalar Tau_d[3], CeedScalar dY[5]) { 182b89d87eSLeila Ghaffari dY[0] = Tau_d[0] * Y[0]; 192b89d87eSLeila Ghaffari dY[1] = Tau_d[1] * Y[1]; 202b89d87eSLeila Ghaffari dY[2] = Tau_d[1] * Y[2]; 212b89d87eSLeila Ghaffari dY[3] = Tau_d[1] * Y[3]; 222b89d87eSLeila Ghaffari dY[4] = Tau_d[2] * Y[4]; 232b89d87eSLeila Ghaffari } 242b89d87eSLeila Ghaffari 252b89d87eSLeila Ghaffari // ***************************************************************************** 262b89d87eSLeila Ghaffari // Helper functions for computing the stabilization terms 272b89d87eSLeila Ghaffari // ***************************************************************************** 288c3b32bfSJames Wright CEED_QFUNCTION_HELPER void StabilizationMatrix(NewtonianIdealGasContext gas, State s, CeedScalar Tau_d[3], CeedScalar strong_residual[5], 298c3b32bfSJames Wright CeedScalar stab[5][3]) { 302b89d87eSLeila Ghaffari CeedScalar dY[5]; 312b89d87eSLeila Ghaffari StateConservative dF[3]; 322b89d87eSLeila Ghaffari // Zero stab so all future terms can safely sum into it 332b730f8bSJeremy L Thompson for (CeedInt i = 0; i < 5; i++) { 342b730f8bSJeremy L Thompson for (CeedInt j = 0; j < 3; j++) stab[i][j] = 0; 352b730f8bSJeremy L Thompson } 368c3b32bfSJames Wright dYFromTau(strong_residual, Tau_d, dY); 373bd61617SKenneth E. Jansen State ds = StateFromY_fwd(gas, s, dY); 382b89d87eSLeila Ghaffari FluxInviscid_fwd(gas, s, ds, dF); 392b89d87eSLeila Ghaffari for (CeedInt i = 0; i < 3; i++) { 402b89d87eSLeila Ghaffari CeedScalar dF_i[5]; 412b89d87eSLeila Ghaffari UnpackState_U(dF[i], dF_i); 422b730f8bSJeremy L Thompson for (CeedInt j = 0; j < 5; j++) stab[j][i] += dF_i[j]; 432b89d87eSLeila Ghaffari } 442b89d87eSLeila Ghaffari } 452b89d87eSLeila Ghaffari 462b730f8bSJeremy L Thompson CEED_QFUNCTION_HELPER void Stabilization(NewtonianIdealGasContext gas, State s, CeedScalar Tau_d[3], State ds[3], CeedScalar U_dot[5], 473bd61617SKenneth E. Jansen const CeedScalar body_force[5], CeedScalar stab[5][3]) { 482b89d87eSLeila Ghaffari // -- Stabilization method: none (Galerkin), SU, or SUPG 498c3b32bfSJames Wright CeedScalar strong_residual[5] = {0}; 502b89d87eSLeila Ghaffari switch (gas->stabilization) { 512b89d87eSLeila Ghaffari case STAB_NONE: 522b89d87eSLeila Ghaffari break; 532b89d87eSLeila Ghaffari case STAB_SU: 548c3b32bfSJames Wright FluxInviscidStrong(gas, s, ds, strong_residual); 552b89d87eSLeila Ghaffari break; 562b89d87eSLeila Ghaffari case STAB_SUPG: 578c3b32bfSJames Wright FluxInviscidStrong(gas, s, ds, strong_residual); 588c3b32bfSJames Wright for (CeedInt j = 0; j < 5; j++) strong_residual[j] += U_dot[j] - body_force[j]; 592b89d87eSLeila Ghaffari break; 602b89d87eSLeila Ghaffari } 618c3b32bfSJames Wright StabilizationMatrix(gas, s, Tau_d, strong_residual, stab); 622b89d87eSLeila Ghaffari } 632b89d87eSLeila Ghaffari 642b89d87eSLeila Ghaffari // ***************************************************************************** 652b89d87eSLeila Ghaffari // Helper function for computing Tau elements (stabilization constant) 662b89d87eSLeila Ghaffari // Model from: 672b89d87eSLeila Ghaffari // PHASTA 682b89d87eSLeila Ghaffari // 692b89d87eSLeila Ghaffari // Tau[i] = itau=0 which is diagonal-Shakib (3 values still but not spatial) 702b89d87eSLeila Ghaffari // ***************************************************************************** 712b730f8bSJeremy L Thompson CEED_QFUNCTION_HELPER void Tau_diagPrim(NewtonianIdealGasContext gas, State s, const CeedScalar dXdx[3][3], const CeedScalar dt, 722b730f8bSJeremy L Thompson CeedScalar Tau_d[3]) { 732b89d87eSLeila Ghaffari // Context 742b89d87eSLeila Ghaffari const CeedScalar Ctau_t = gas->Ctau_t; 752b89d87eSLeila Ghaffari const CeedScalar Ctau_v = gas->Ctau_v; 762b89d87eSLeila Ghaffari const CeedScalar Ctau_C = gas->Ctau_C; 772b89d87eSLeila Ghaffari const CeedScalar Ctau_M = gas->Ctau_M; 782b89d87eSLeila Ghaffari const CeedScalar Ctau_E = gas->Ctau_E; 792b89d87eSLeila Ghaffari const CeedScalar cv = gas->cv; 802b89d87eSLeila Ghaffari const CeedScalar mu = gas->mu; 812b89d87eSLeila Ghaffari const CeedScalar rho = s.U.density; 822b89d87eSLeila Ghaffari 832b89d87eSLeila Ghaffari CeedScalar tau; 842b89d87eSLeila Ghaffari CeedScalar dts; 852b89d87eSLeila Ghaffari CeedScalar fact; 862b89d87eSLeila Ghaffari 87b9b033b3SJames Wright CeedScalar gijd_mat[3][3] = {{0.}}, velocity_term; 88b9b033b3SJames Wright MatMat3(dXdx, dXdx, CEED_TRANSPOSE, CEED_NOTRANSPOSE, gijd_mat); 892b89d87eSLeila Ghaffari 902b89d87eSLeila Ghaffari dts = Ctau_t / dt; 912b89d87eSLeila Ghaffari 92b9b033b3SJames Wright { // u_i g_ij u_j 93b9b033b3SJames Wright CeedScalar gij_uj[3] = {0.}; 94b9b033b3SJames Wright MatVec3(gijd_mat, s.Y.velocity, CEED_NOTRANSPOSE, gij_uj); 95b9b033b3SJames Wright velocity_term = Dot3(s.Y.velocity, gij_uj); 96b9b033b3SJames Wright } 97b9b033b3SJames Wright 98b9b033b3SJames Wright tau = Square(rho) * (4. * Square(dts) + velocity_term) + Ctau_v * Square(mu) * DotN((CeedScalar *)gijd_mat, (CeedScalar *)gijd_mat, 9); 992b89d87eSLeila Ghaffari 1002b89d87eSLeila Ghaffari fact = sqrt(tau); 1012b89d87eSLeila Ghaffari 102b9b033b3SJames Wright Tau_d[0] = Ctau_C * fact / (rho * (gijd_mat[0][0] + gijd_mat[1][1] + gijd_mat[2][2])) * 0.125; 1032b89d87eSLeila Ghaffari Tau_d[1] = Ctau_M / fact; 1042b89d87eSLeila Ghaffari Tau_d[2] = Ctau_E / (fact * cv); 1052b89d87eSLeila Ghaffari 106ea61e9acSJeremy L Thompson // consider putting back the way I initially had it 107ea61e9acSJeremy 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 1082b89d87eSLeila Ghaffari // but in that case energy tau is scaled by the product of Ctau_E * Ctau_M 109ea61e9acSJeremy 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 1102b89d87eSLeila Ghaffari // Ctau_v * mu * mu IF AND ONLY IF we don't add viscosity law =f(T) 1112b89d87eSLeila Ghaffari } 112