1727da7e7SJeremy L Thompson // Copyright (c) 2017-2022, Lawrence Livermore National Security, LLC and other CEED contributors. 2727da7e7SJeremy L Thompson // All Rights Reserved. See the top-level LICENSE and NOTICE files for details. 33a8779fbSJames Wright // 4727da7e7SJeremy L Thompson // SPDX-License-Identifier: BSD-2-Clause 53a8779fbSJames Wright // 6727da7e7SJeremy L Thompson // This file is part of CEED: http://github.com/ceed 73a8779fbSJames Wright 83a8779fbSJames Wright /// @file 93a8779fbSJames Wright /// Operator for Navier-Stokes example using PETSc 103a8779fbSJames Wright 113a8779fbSJames Wright 123a8779fbSJames Wright #ifndef newtonian_h 133a8779fbSJames Wright #define newtonian_h 143a8779fbSJames Wright 153a8779fbSJames Wright #include <math.h> 163a8779fbSJames Wright #include <ceed.h> 1715a3537eSJed Brown #include "newtonian_types.h" 183a8779fbSJames Wright 193a8779fbSJames Wright #ifndef M_PI 203a8779fbSJames Wright #define M_PI 3.14159265358979323846 213a8779fbSJames Wright #endif 223a8779fbSJames Wright 23c1a52365SJed Brown typedef struct { 24c1a52365SJed Brown CeedScalar pressure; 25c1a52365SJed Brown CeedScalar velocity[3]; 26c1a52365SJed Brown CeedScalar temperature; 27c1a52365SJed Brown } StatePrimitive; 28c1a52365SJed Brown 29c1a52365SJed Brown typedef struct { 30c1a52365SJed Brown CeedScalar density; 31c1a52365SJed Brown CeedScalar momentum[3]; 32c1a52365SJed Brown CeedScalar E_total; 33c1a52365SJed Brown } StateConservative; 34c1a52365SJed Brown 35c1a52365SJed Brown typedef struct { 36c1a52365SJed Brown StateConservative U; 37c1a52365SJed Brown StatePrimitive Y; 38c1a52365SJed Brown } State; 39c1a52365SJed Brown 40c1a52365SJed Brown CEED_QFUNCTION_HELPER CeedScalar Dot3(const CeedScalar u[3], 41c1a52365SJed Brown const CeedScalar v[3]) { 42c1a52365SJed Brown return u[0]*v[0] + u[1]*v[1] + u[2]*v[2]; 43c1a52365SJed Brown } 44c1a52365SJed Brown 45c1a52365SJed Brown CEED_QFUNCTION_HELPER StatePrimitive StatePrimitiveFromConservative( 46c1a52365SJed Brown NewtonianIdealGasContext gas, StateConservative U, const CeedScalar x[3]) { 47c1a52365SJed Brown StatePrimitive Y; 48c1a52365SJed Brown for (int i=0; i<3; i++) Y.velocity[i] = U.momentum[i] / U.density; 49c1a52365SJed Brown CeedScalar e_kinetic = .5 * Dot3(Y.velocity, Y.velocity); 50c1a52365SJed Brown CeedScalar e_potential = -Dot3(gas->g, x); 51c1a52365SJed Brown CeedScalar e_total = U.E_total / U.density; 52c1a52365SJed Brown CeedScalar e_internal = e_total - e_kinetic - e_potential; 53c1a52365SJed Brown Y.temperature = e_internal / gas->cv; 54c1a52365SJed Brown Y.pressure = (gas->cp / gas->cv - 1) * U.density * e_internal; 55c1a52365SJed Brown return Y; 56c1a52365SJed Brown } 57c1a52365SJed Brown 58c1a52365SJed Brown CEED_QFUNCTION_HELPER StatePrimitive StatePrimitiveFromConservative_fwd( 59c1a52365SJed Brown NewtonianIdealGasContext gas, State s, StateConservative dU, 60c1a52365SJed Brown const CeedScalar x[3], const CeedScalar dx[3]) { 61c1a52365SJed Brown StatePrimitive dY; 62c1a52365SJed Brown for (int i=0; i<3; i++) { 63c1a52365SJed Brown dY.velocity[i] = (dU.momentum[i] - s.Y.velocity[i] * dU.density) / s.U.density; 64c1a52365SJed Brown } 65c1a52365SJed Brown CeedScalar e_kinetic = .5 * Dot3(s.Y.velocity, s.Y.velocity); 66c1a52365SJed Brown CeedScalar de_kinetic = Dot3(dY.velocity, s.Y.velocity); 67c1a52365SJed Brown CeedScalar e_potential = -Dot3(gas->g, x); 68c1a52365SJed Brown CeedScalar de_potential = -Dot3(gas->g, dx); 69c1a52365SJed Brown CeedScalar e_total = s.U.E_total / s.U.density; 70c1a52365SJed Brown CeedScalar de_total = (dU.E_total - e_total * dU.density) / s.U.density; 71c1a52365SJed Brown CeedScalar e_internal = e_total - e_kinetic - e_potential; 72c1a52365SJed Brown CeedScalar de_internal = de_total - de_kinetic - de_potential; 73c1a52365SJed Brown dY.temperature = de_internal / gas->cv; 74c1a52365SJed Brown dY.pressure = (gas->cp / gas->cv - 1) 75c1a52365SJed Brown * (dU.density * e_internal + s.U.density * de_internal); 76c1a52365SJed Brown return dY; 77c1a52365SJed Brown } 78c1a52365SJed Brown 79c1a52365SJed Brown CEED_QFUNCTION_HELPER State StateFromU(NewtonianIdealGasContext gas, 80c1a52365SJed Brown const CeedScalar U[5], const CeedScalar x[3]) { 81c1a52365SJed Brown State s; 82c1a52365SJed Brown s.U.density = U[0]; 83c1a52365SJed Brown s.U.momentum[0] = U[1]; 84c1a52365SJed Brown s.U.momentum[1] = U[2]; 85c1a52365SJed Brown s.U.momentum[2] = U[3]; 86c1a52365SJed Brown s.U.E_total = U[4]; 87c1a52365SJed Brown s.Y = StatePrimitiveFromConservative(gas, s.U, x); 88c1a52365SJed Brown return s; 89c1a52365SJed Brown } 90c1a52365SJed Brown 912f7ce6c1SJed Brown CEED_QFUNCTION_HELPER State StateFromU_fwd(NewtonianIdealGasContext gas, 922f7ce6c1SJed Brown State s, const CeedScalar dU[5], 932f7ce6c1SJed Brown const CeedScalar x[3], const CeedScalar dx[3]) { 942f7ce6c1SJed Brown State ds; 952f7ce6c1SJed Brown ds.U.density = dU[0]; 962f7ce6c1SJed Brown ds.U.momentum[0] = dU[1]; 972f7ce6c1SJed Brown ds.U.momentum[1] = dU[2]; 982f7ce6c1SJed Brown ds.U.momentum[2] = dU[3]; 992f7ce6c1SJed Brown ds.U.E_total = dU[4]; 1002f7ce6c1SJed Brown ds.Y = StatePrimitiveFromConservative_fwd(gas, s, ds.U, x, dx); 1012f7ce6c1SJed Brown return ds; 1022f7ce6c1SJed Brown } 1032f7ce6c1SJed Brown 104c1a52365SJed Brown CEED_QFUNCTION_HELPER void FluxInviscid(NewtonianIdealGasContext gas, State s, 105c1a52365SJed Brown StateConservative Flux[3]) { 106c1a52365SJed Brown for (int i=0; i<3; i++) { 107c1a52365SJed Brown Flux[i].density = s.U.momentum[i]; 108c1a52365SJed Brown for (int j=0; j<3; j++) 109c1a52365SJed Brown Flux[i].momentum[j] = s.U.momentum[i] * s.Y.velocity[j] 110c1a52365SJed Brown + s.Y.pressure * (i == j); 111c1a52365SJed Brown Flux[i].E_total = (s.U.E_total + s.Y.pressure) * s.Y.velocity[i]; 112c1a52365SJed Brown } 113c1a52365SJed Brown } 114c1a52365SJed Brown 115c1a52365SJed Brown CEED_QFUNCTION_HELPER void FluxInviscid_fwd(NewtonianIdealGasContext gas, 116c1a52365SJed Brown State s, State ds, StateConservative dFlux[3]) { 117c1a52365SJed Brown for (int i=0; i<3; i++) { 118c1a52365SJed Brown dFlux[i].density = ds.U.momentum[i]; 119c1a52365SJed Brown for (int j=0; j<3; j++) 120c1a52365SJed Brown dFlux[i].momentum[j] = ds.U.momentum[i] * s.Y.velocity[j] + 121c1a52365SJed Brown s.U.momentum[i] * ds.Y.velocity[j] + ds.Y.pressure * (i == j); 122c1a52365SJed Brown dFlux[i].E_total = (ds.U.E_total + ds.Y.pressure) * s.Y.velocity[i] + 123c1a52365SJed Brown (s.U.E_total + s.Y.pressure) * ds.Y.velocity[i]; 124c1a52365SJed Brown } 125c1a52365SJed Brown } 126c1a52365SJed Brown 127c1a52365SJed Brown // Kelvin-Mandel notation 128c1a52365SJed Brown CEED_QFUNCTION_HELPER void KMStrainRate(const State grad_s[3], 129c1a52365SJed Brown CeedScalar strain_rate[6]) { 130c1a52365SJed Brown const CeedScalar weight = 1 / sqrt(2.); 131c1a52365SJed Brown strain_rate[0] = grad_s[0].Y.velocity[0]; 132c1a52365SJed Brown strain_rate[1] = grad_s[1].Y.velocity[1]; 133c1a52365SJed Brown strain_rate[2] = grad_s[2].Y.velocity[2]; 134c1a52365SJed Brown strain_rate[3] = weight * (grad_s[2].Y.velocity[1] + grad_s[1].Y.velocity[2]); 135c1a52365SJed Brown strain_rate[4] = weight * (grad_s[2].Y.velocity[0] + grad_s[0].Y.velocity[2]); 136c1a52365SJed Brown strain_rate[5] = weight * (grad_s[1].Y.velocity[0] + grad_s[0].Y.velocity[1]); 137c1a52365SJed Brown } 138c1a52365SJed Brown 139c1a52365SJed Brown CEED_QFUNCTION_HELPER void KMUnpack(const CeedScalar v[6], CeedScalar A[3][3]) { 140c1a52365SJed Brown const CeedScalar weight = 1 / sqrt(2.); 141c1a52365SJed Brown A[0][0] = v[0]; 142c1a52365SJed Brown A[1][1] = v[1]; 143c1a52365SJed Brown A[2][2] = v[2]; 144c1a52365SJed Brown A[2][1] = A[1][2] = weight * v[3]; 145c1a52365SJed Brown A[2][0] = A[0][2] = weight * v[4]; 146c1a52365SJed Brown A[1][0] = A[0][1] = weight * v[5]; 147c1a52365SJed Brown } 148c1a52365SJed Brown 149c1a52365SJed Brown CEED_QFUNCTION_HELPER void NewtonianStress(NewtonianIdealGasContext gas, 150c1a52365SJed Brown const CeedScalar strain_rate[6], CeedScalar stress[6]) { 151c1a52365SJed Brown CeedScalar div_u = strain_rate[0] + strain_rate[1] + strain_rate[2]; 152c1a52365SJed Brown for (int i=0; i<6; i++) { 153c1a52365SJed Brown stress[i] = gas->mu * (2 * strain_rate[i] + gas->lambda * div_u * (i < 3)); 154c1a52365SJed Brown } 155c1a52365SJed Brown } 156c1a52365SJed Brown 157c1a52365SJed Brown CEED_QFUNCTION_HELPER void ViscousEnergyFlux(NewtonianIdealGasContext gas, 158c1a52365SJed Brown StatePrimitive Y, const State grad_s[3], const CeedScalar stress[3][3], 159c1a52365SJed Brown CeedScalar Fe[3]) { 160c1a52365SJed Brown for (int i=0; i<3; i++) { 161c1a52365SJed Brown Fe[i] = - Y.velocity[0] * stress[0][i] 162c1a52365SJed Brown - Y.velocity[1] * stress[1][i] 163c1a52365SJed Brown - Y.velocity[2] * stress[2][i] 164c1a52365SJed Brown - gas->k * grad_s[i].Y.temperature; 165c1a52365SJed Brown } 166c1a52365SJed Brown } 167c1a52365SJed Brown 1683a8779fbSJames Wright // ***************************************************************************** 1693a8779fbSJames Wright // Helper function for computing flux Jacobian 1703a8779fbSJames Wright // ***************************************************************************** 1713a8779fbSJames Wright CEED_QFUNCTION_HELPER void computeFluxJacobian_NS(CeedScalar dF[3][5][5], 1723a8779fbSJames Wright const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 173bb8a0c61SJames Wright const CeedScalar gamma, const CeedScalar g[3], const CeedScalar x[3]) { 1743a8779fbSJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; // Velocity square 175bb8a0c61SJames Wright CeedScalar e_potential = -(g[0]*x[0] + g[1]*x[1] + g[2]*x[2]); 1763a8779fbSJames Wright for (CeedInt i=0; i<3; i++) { // Jacobian matrices for 3 directions 1773a8779fbSJames Wright for (CeedInt j=0; j<3; j++) { // Rows of each Jacobian matrix 178bb8a0c61SJames Wright dF[i][j+1][0] = ((i==j) ? ((gamma-1.)*(u_sq/2. - e_potential)) : 0.) - 179bb8a0c61SJames Wright u[i]*u[j]; 1803a8779fbSJames Wright for (CeedInt k=0; k<3; k++) { // Columns of each Jacobian matrix 1813a8779fbSJames Wright dF[i][0][k+1] = ((i==k) ? 1. : 0.); 1823a8779fbSJames Wright dF[i][j+1][k+1] = ((j==k) ? u[i] : 0.) + 1833a8779fbSJames Wright ((i==k) ? u[j] : 0.) - 1843a8779fbSJames Wright ((i==j) ? u[k] : 0.) * (gamma-1.); 1853a8779fbSJames Wright dF[i][4][k+1] = ((i==k) ? (E*gamma/rho - (gamma-1.)*u_sq/2.) : 0.) - 1863a8779fbSJames Wright (gamma-1.)*u[i]*u[k]; 1873a8779fbSJames Wright } 1883a8779fbSJames Wright dF[i][j+1][4] = ((i==j) ? (gamma-1.) : 0.); 1893a8779fbSJames Wright } 1903a8779fbSJames Wright dF[i][4][0] = u[i] * ((gamma-1.)*u_sq - E*gamma/rho); 1913a8779fbSJames Wright dF[i][4][4] = u[i] * gamma; 1923a8779fbSJames Wright } 1933a8779fbSJames Wright } 1943a8779fbSJames Wright 1953a8779fbSJames Wright // ***************************************************************************** 196bb8a0c61SJames Wright // Helper function for computing flux Jacobian of Primitive variables 197bb8a0c61SJames Wright // ***************************************************************************** 198bb8a0c61SJames Wright CEED_QFUNCTION_HELPER void computeFluxJacobian_NSp(CeedScalar dF[3][5][5], 199bb8a0c61SJames Wright const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 200bb8a0c61SJames Wright const CeedScalar Rd, const CeedScalar cv) { 201bb8a0c61SJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; // Velocity square 202bb8a0c61SJames Wright // TODO Add in gravity's contribution 203bb8a0c61SJames Wright 204bb8a0c61SJames Wright CeedScalar T = ( E / rho - u_sq / 2. ) / cv; 205bb8a0c61SJames Wright CeedScalar drdT = -rho / T; 206bb8a0c61SJames Wright CeedScalar drdP = 1. / ( Rd * T); 207bb8a0c61SJames Wright CeedScalar etot = E / rho ; 208bb8a0c61SJames Wright CeedScalar e2p = drdP * etot + 1. ; 209bb8a0c61SJames Wright CeedScalar e3p = ( E + rho * Rd * T ); 210bb8a0c61SJames Wright CeedScalar e4p = drdT * etot + rho * cv ; 211bb8a0c61SJames Wright 212bb8a0c61SJames Wright for (CeedInt i=0; i<3; i++) { // Jacobian matrices for 3 directions 213bb8a0c61SJames Wright for (CeedInt j=0; j<3; j++) { // j counts F^{m_j} 214bb8a0c61SJames Wright // [row][col] of A_i 215bb8a0c61SJames Wright dF[i][j+1][0] = drdP * u[i] * u[j] + ((i==j) ? 1. : 0.); // F^{{m_j} wrt p 216bb8a0c61SJames Wright for (CeedInt k=0; k<3; k++) { // k counts the wrt vel_k 2172acc7cbcSKenneth E. Jansen dF[i][0][k+1] = ((i==k) ? rho : 0.); // F^c wrt u_k 218bb8a0c61SJames Wright dF[i][j+1][k+1] = (((j==k) ? u[i] : 0.) + // F^m_j wrt u_k 219bb8a0c61SJames Wright ((i==k) ? u[j] : 0.) ) * rho; 220bb8a0c61SJames Wright dF[i][4][k+1] = rho * u[i] * u[k] 221bb8a0c61SJames Wright + ((i==k) ? e3p : 0.) ; // F^e wrt u_k 222bb8a0c61SJames Wright } 223bb8a0c61SJames Wright dF[i][j+1][4] = drdT * u[i] * u[j]; // F^{m_j} wrt T 224bb8a0c61SJames Wright } 225bb8a0c61SJames Wright dF[i][4][0] = u[i] * e2p; // F^e wrt p 226bb8a0c61SJames Wright dF[i][4][4] = u[i] * e4p; // F^e wrt T 227bb8a0c61SJames Wright dF[i][0][0] = u[i] * drdP; // F^c wrt p 228bb8a0c61SJames Wright dF[i][0][4] = u[i] * drdT; // F^c wrt T 229bb8a0c61SJames Wright } 230bb8a0c61SJames Wright } 231bb8a0c61SJames Wright 232bb8a0c61SJames Wright CEED_QFUNCTION_HELPER void PrimitiveToConservative_fwd(const CeedScalar rho, 233bb8a0c61SJames Wright const CeedScalar u[3], const CeedScalar E, const CeedScalar Rd, 234bb8a0c61SJames Wright const CeedScalar cv, const CeedScalar dY[5], CeedScalar dU[5]) { 235bb8a0c61SJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; 236bb8a0c61SJames Wright CeedScalar T = ( E / rho - u_sq / 2. ) / cv; 237bb8a0c61SJames Wright CeedScalar drdT = -rho / T; 238bb8a0c61SJames Wright CeedScalar drdP = 1. / ( Rd * T); 239bb8a0c61SJames Wright dU[0] = drdP * dY[0] + drdT * dY[4]; 240bb8a0c61SJames Wright CeedScalar de_kinetic = 0; 241bb8a0c61SJames Wright for (int i=0; i<3; i++) { 242bb8a0c61SJames Wright dU[1+i] = dU[0] * u[i] + rho * dY[1+i]; 243bb8a0c61SJames Wright de_kinetic += u[i] * dY[1+i]; 244bb8a0c61SJames Wright } 245bb8a0c61SJames Wright dU[4] = rho * cv * dY[4] + dU[0] * cv * T // internal energy: rho * e 246bb8a0c61SJames Wright + rho * de_kinetic + .5 * dU[0] * u_sq; // kinetic energy: .5 * rho * |u|^2 247bb8a0c61SJames Wright } 248bb8a0c61SJames Wright 249bb8a0c61SJames Wright // ***************************************************************************** 250bb8a0c61SJames Wright // Helper function for computing Tau elements (stabilization constant) 251bb8a0c61SJames Wright // Model from: 252bb8a0c61SJames Wright // PHASTA 253bb8a0c61SJames Wright // 254bb8a0c61SJames Wright // Tau[i] = itau=0 which is diagonal-Shakib (3 values still but not spatial) 255bb8a0c61SJames Wright // 256bb8a0c61SJames Wright // Where NOT UPDATED YET 257bb8a0c61SJames Wright // ***************************************************************************** 258bb8a0c61SJames Wright CEED_QFUNCTION_HELPER void Tau_diagPrim(CeedScalar Tau_d[3], 259bb8a0c61SJames Wright const CeedScalar dXdx[3][3], const CeedScalar u[3], 260bb8a0c61SJames Wright const CeedScalar cv, const NewtonianIdealGasContext newt_ctx, 261bb8a0c61SJames Wright const CeedScalar mu, const CeedScalar dt, 262bb8a0c61SJames Wright const CeedScalar rho) { 263bb8a0c61SJames Wright // Context 264bb8a0c61SJames Wright const CeedScalar Ctau_t = newt_ctx->Ctau_t; 265bb8a0c61SJames Wright const CeedScalar Ctau_v = newt_ctx->Ctau_v; 266bb8a0c61SJames Wright const CeedScalar Ctau_C = newt_ctx->Ctau_C; 267bb8a0c61SJames Wright const CeedScalar Ctau_M = newt_ctx->Ctau_M; 268bb8a0c61SJames Wright const CeedScalar Ctau_E = newt_ctx->Ctau_E; 269bb8a0c61SJames Wright CeedScalar gijd[6]; 270bb8a0c61SJames Wright CeedScalar tau; 271bb8a0c61SJames Wright CeedScalar dts; 272bb8a0c61SJames Wright CeedScalar fact; 273bb8a0c61SJames Wright 274bb8a0c61SJames Wright //*INDENT-OFF* 275bb8a0c61SJames Wright gijd[0] = dXdx[0][0] * dXdx[0][0] 276bb8a0c61SJames Wright + dXdx[1][0] * dXdx[1][0] 277bb8a0c61SJames Wright + dXdx[2][0] * dXdx[2][0]; 278bb8a0c61SJames Wright 279bb8a0c61SJames Wright gijd[1] = dXdx[0][0] * dXdx[0][1] 280bb8a0c61SJames Wright + dXdx[1][0] * dXdx[1][1] 281bb8a0c61SJames Wright + dXdx[2][0] * dXdx[2][1]; 282bb8a0c61SJames Wright 283bb8a0c61SJames Wright gijd[2] = dXdx[0][1] * dXdx[0][1] 284bb8a0c61SJames Wright + dXdx[1][1] * dXdx[1][1] 285bb8a0c61SJames Wright + dXdx[2][1] * dXdx[2][1]; 286bb8a0c61SJames Wright 287bb8a0c61SJames Wright gijd[3] = dXdx[0][0] * dXdx[0][2] 288bb8a0c61SJames Wright + dXdx[1][0] * dXdx[1][2] 289bb8a0c61SJames Wright + dXdx[2][0] * dXdx[2][2]; 290bb8a0c61SJames Wright 291bb8a0c61SJames Wright gijd[4] = dXdx[0][1] * dXdx[0][2] 292bb8a0c61SJames Wright + dXdx[1][1] * dXdx[1][2] 293bb8a0c61SJames Wright + dXdx[2][1] * dXdx[2][2]; 294bb8a0c61SJames Wright 295bb8a0c61SJames Wright gijd[5] = dXdx[0][2] * dXdx[0][2] 296bb8a0c61SJames Wright + dXdx[1][2] * dXdx[1][2] 297bb8a0c61SJames Wright + dXdx[2][2] * dXdx[2][2]; 298bb8a0c61SJames Wright //*INDENT-ON* 299bb8a0c61SJames Wright 300bb8a0c61SJames Wright dts = Ctau_t / dt ; 301bb8a0c61SJames Wright 302bb8a0c61SJames Wright tau = rho*rho*((4. * dts * dts) 303bb8a0c61SJames Wright + u[0] * ( u[0] * gijd[0] + 2. * ( u[1] * gijd[1] + u[2] * gijd[3])) 304bb8a0c61SJames Wright + u[1] * ( u[1] * gijd[2] + 2. * u[2] * gijd[4]) 305bb8a0c61SJames Wright + u[2] * u[2] * gijd[5]) 306bb8a0c61SJames Wright + Ctau_v* mu * mu * 307bb8a0c61SJames Wright (gijd[0]*gijd[0] + gijd[2]*gijd[2] + gijd[5]*gijd[5] + 308bb8a0c61SJames Wright + 2. * (gijd[1]*gijd[1] + gijd[3]*gijd[3] + gijd[4]*gijd[4])); 309bb8a0c61SJames Wright 310bb8a0c61SJames Wright fact=sqrt(tau); 311bb8a0c61SJames Wright 312bb8a0c61SJames Wright Tau_d[0] = Ctau_C * fact / (rho*(gijd[0] + gijd[2] + gijd[5]))*0.125; 313bb8a0c61SJames Wright 314bb8a0c61SJames Wright Tau_d[1] = Ctau_M / fact; 315bb8a0c61SJames Wright Tau_d[2] = Ctau_E / ( fact * cv ); 316bb8a0c61SJames Wright 317bb8a0c61SJames Wright // consider putting back the way I initially had it Ctau_E * Tau_d[1] /cv 318bb8a0c61SJames Wright // to avoid a division if the compiler is smart enough to see that cv IS 319bb8a0c61SJames Wright // a constant that it could invert once for all elements 320bb8a0c61SJames Wright // but in that case energy tau is scaled by the product of Ctau_E * Ctau_M 321bb8a0c61SJames Wright // OR we could absorb cv into Ctau_E but this puts more burden on user to 322bb8a0c61SJames Wright // know how to change constants with a change of fluid or units. Same for 323bb8a0c61SJames Wright // Ctau_v * mu * mu IF AND ONLY IF we don't add viscosity law =f(T) 324bb8a0c61SJames Wright } 325bb8a0c61SJames Wright 326bb8a0c61SJames Wright // ***************************************************************************** 3273a8779fbSJames Wright // This QFunction sets a "still" initial condition for generic Newtonian IG problems 3283a8779fbSJames Wright // ***************************************************************************** 3293a8779fbSJames Wright CEED_QFUNCTION(ICsNewtonianIG)(void *ctx, CeedInt Q, 3303a8779fbSJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 3313a8779fbSJames Wright // Inputs 3323a8779fbSJames Wright const CeedScalar (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 3333a8779fbSJames Wright 3343a8779fbSJames Wright // Outputs 3353a8779fbSJames Wright CeedScalar (*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 3363a8779fbSJames Wright 337bb8a0c61SJames Wright // Context 338bb8a0c61SJames Wright const SetupContext context = (SetupContext)ctx; 339bb8a0c61SJames Wright const CeedScalar theta0 = context->theta0; 340bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 341bb8a0c61SJames Wright const CeedScalar cv = context->cv; 342bb8a0c61SJames Wright const CeedScalar cp = context->cp; 343bb8a0c61SJames Wright const CeedScalar *g = context->g; 344bb8a0c61SJames Wright const CeedScalar Rd = cp - cv; 345bb8a0c61SJames Wright 3463a8779fbSJames Wright // Quadrature Point Loop 3473a8779fbSJames Wright CeedPragmaSIMD 3483a8779fbSJames Wright for (CeedInt i=0; i<Q; i++) { 3493a8779fbSJames Wright CeedScalar q[5] = {0.}; 3503a8779fbSJames Wright 3513a8779fbSJames Wright // Setup 3523a8779fbSJames Wright // -- Coordinates 353bb8a0c61SJames Wright const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 354bb8a0c61SJames Wright const CeedScalar e_potential = -(g[0]*x[0] + g[1]*x[1] + g[2]*x[2]); 3553a8779fbSJames Wright 3563a8779fbSJames Wright // -- Density 357bb8a0c61SJames Wright const CeedScalar rho = P0 / (Rd*theta0); 3583a8779fbSJames Wright 3593a8779fbSJames Wright // Initial Conditions 3603a8779fbSJames Wright q[0] = rho; 3613a8779fbSJames Wright q[1] = 0.0; 3623a8779fbSJames Wright q[2] = 0.0; 3633a8779fbSJames Wright q[3] = 0.0; 364bb8a0c61SJames Wright q[4] = rho * (cv*theta0 + e_potential); 3653a8779fbSJames Wright 3663a8779fbSJames Wright for (CeedInt j=0; j<5; j++) 3673a8779fbSJames Wright q0[j][i] = q[j]; 3683a8779fbSJames Wright } // End of Quadrature Point Loop 3693a8779fbSJames Wright return 0; 3703a8779fbSJames Wright } 3713a8779fbSJames Wright 3723a8779fbSJames Wright // ***************************************************************************** 3733a8779fbSJames Wright // This QFunction implements the following formulation of Navier-Stokes with 3743a8779fbSJames Wright // explicit time stepping method 3753a8779fbSJames Wright // 3763a8779fbSJames Wright // This is 3D compressible Navier-Stokes in conservation form with state 3773a8779fbSJames Wright // variables of density, momentum density, and total energy density. 3783a8779fbSJames Wright // 3793a8779fbSJames Wright // State Variables: q = ( rho, U1, U2, U3, E ) 3803a8779fbSJames Wright // rho - Mass Density 3813a8779fbSJames Wright // Ui - Momentum Density, Ui = rho ui 3823a8779fbSJames Wright // E - Total Energy Density, E = rho (cv T + (u u)/2 + g z) 3833a8779fbSJames Wright // 3843a8779fbSJames Wright // Navier-Stokes Equations: 3853a8779fbSJames Wright // drho/dt + div( U ) = 0 3863a8779fbSJames Wright // dU/dt + div( rho (u x u) + P I3 ) + rho g khat = div( Fu ) 3873a8779fbSJames Wright // dE/dt + div( (E + P) u ) = div( Fe ) 3883a8779fbSJames Wright // 3893a8779fbSJames Wright // Viscous Stress: 3903a8779fbSJames Wright // Fu = mu (grad( u ) + grad( u )^T + lambda div ( u ) I3) 3913a8779fbSJames Wright // 3923a8779fbSJames Wright // Thermal Stress: 3933a8779fbSJames Wright // Fe = u Fu + k grad( T ) 394bb8a0c61SJames Wright // Equation of State 3953a8779fbSJames Wright // P = (gamma - 1) (E - rho (u u) / 2 - rho g z) 3963a8779fbSJames Wright // 3973a8779fbSJames Wright // Stabilization: 3983a8779fbSJames Wright // Tau = diag(TauC, TauM, TauM, TauM, TauE) 3993a8779fbSJames Wright // f1 = rho sqrt(ui uj gij) 4003a8779fbSJames Wright // gij = dXi/dX * dXi/dX 4013a8779fbSJames Wright // TauC = Cc f1 / (8 gii) 4023a8779fbSJames Wright // TauM = min( 1 , 1 / f1 ) 4033a8779fbSJames Wright // TauE = TauM / (Ce cv) 4043a8779fbSJames Wright // 4053a8779fbSJames Wright // SU = Galerkin + grad(v) . ( Ai^T * Tau * (Aj q,j) ) 4063a8779fbSJames Wright // 4073a8779fbSJames Wright // Constants: 4083a8779fbSJames Wright // lambda = - 2 / 3, From Stokes hypothesis 4093a8779fbSJames Wright // mu , Dynamic viscosity 4103a8779fbSJames Wright // k , Thermal conductivity 4113a8779fbSJames Wright // cv , Specific heat, constant volume 4123a8779fbSJames Wright // cp , Specific heat, constant pressure 4133a8779fbSJames Wright // g , Gravity 4143a8779fbSJames Wright // gamma = cp / cv, Specific heat ratio 4153a8779fbSJames Wright // 4163a8779fbSJames Wright // We require the product of the inverse of the Jacobian (dXdx_j,k) and 4173a8779fbSJames Wright // its transpose (dXdx_k,j) to properly compute integrals of the form: 4183a8779fbSJames Wright // int( gradv gradu ) 4193a8779fbSJames Wright // 4203a8779fbSJames Wright // ***************************************************************************** 421c1a52365SJed Brown CEED_QFUNCTION(RHSFunction_Newtonian)(void *ctx, CeedInt Q, 4223a8779fbSJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 4233a8779fbSJames Wright // *INDENT-OFF* 4243a8779fbSJames Wright // Inputs 4253a8779fbSJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 426*752f40e3SJed Brown (*Grad_q)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 4273a8779fbSJames Wright (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 4283a8779fbSJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 4293a8779fbSJames Wright // Outputs 4303a8779fbSJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 431*752f40e3SJed Brown (*Grad_v)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1]; 4323a8779fbSJames Wright // *INDENT-ON* 4333a8779fbSJames Wright 4343a8779fbSJames Wright // Context 4353a8779fbSJames Wright NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 4363a8779fbSJames Wright const CeedScalar mu = context->mu; 4373a8779fbSJames Wright const CeedScalar cv = context->cv; 4383a8779fbSJames Wright const CeedScalar cp = context->cp; 439bb8a0c61SJames Wright const CeedScalar *g = context->g; 440bb8a0c61SJames Wright const CeedScalar dt = context->dt; 4413a8779fbSJames Wright const CeedScalar gamma = cp / cv; 442bb8a0c61SJames Wright const CeedScalar Rd = cp - cv; 4433a8779fbSJames Wright 4443a8779fbSJames Wright CeedPragmaSIMD 4453a8779fbSJames Wright // Quadrature Point Loop 4463a8779fbSJames Wright for (CeedInt i=0; i<Q; i++) { 447c1a52365SJed Brown CeedScalar U[5]; 448c1a52365SJed Brown for (int j=0; j<5; j++) U[j] = q[j][i]; 449c1a52365SJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 450c1a52365SJed Brown State s = StateFromU(context, U, x_i); 451c1a52365SJed Brown 4523a8779fbSJames Wright // -- Interp-to-Interp q_data 4533a8779fbSJames Wright const CeedScalar wdetJ = q_data[0][i]; 4543a8779fbSJames Wright // -- Interp-to-Grad q_data 4553a8779fbSJames Wright // ---- Inverse of change of coordinate matrix: X_i,j 4563a8779fbSJames Wright // *INDENT-OFF* 4573a8779fbSJames Wright const CeedScalar dXdx[3][3] = {{q_data[1][i], 4583a8779fbSJames Wright q_data[2][i], 4593a8779fbSJames Wright q_data[3][i]}, 4603a8779fbSJames Wright {q_data[4][i], 4613a8779fbSJames Wright q_data[5][i], 4623a8779fbSJames Wright q_data[6][i]}, 4633a8779fbSJames Wright {q_data[7][i], 4643a8779fbSJames Wright q_data[8][i], 4653a8779fbSJames Wright q_data[9][i]} 4663a8779fbSJames Wright }; 4673a8779fbSJames Wright // *INDENT-ON* 4683a8779fbSJames Wright 469c1a52365SJed Brown State grad_s[3]; 470c1a52365SJed Brown for (int j=0; j<3; j++) { 4712f7ce6c1SJed Brown CeedScalar dx_i[3] = {0}, dU[5]; 472*752f40e3SJed Brown for (int k=0; k<5; k++) dU[k] = Grad_q[0][k][i] * dXdx[0][j] 473*752f40e3SJed Brown + Grad_q[1][k][i] * dXdx[1][j] 474*752f40e3SJed Brown + Grad_q[2][k][i] * dXdx[2][j]; 475c1a52365SJed Brown dx_i[j] = 1.; 4762f7ce6c1SJed Brown grad_s[j] = StateFromU_fwd(context, s, dU, x_i, dx_i); 477c1a52365SJed Brown } 478c1a52365SJed Brown 479c1a52365SJed Brown CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 480c1a52365SJed Brown KMStrainRate(grad_s, strain_rate); 481c1a52365SJed Brown NewtonianStress(context, strain_rate, kmstress); 482c1a52365SJed Brown KMUnpack(kmstress, stress); 483c1a52365SJed Brown ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 484c1a52365SJed Brown 485c1a52365SJed Brown StateConservative F_inviscid[3]; 486c1a52365SJed Brown FluxInviscid(context, s, F_inviscid); 487c1a52365SJed Brown 488c1a52365SJed Brown // Total flux 489c1a52365SJed Brown CeedScalar Flux[5][3]; 490c1a52365SJed Brown for (int j=0; j<3; j++) { 491c1a52365SJed Brown Flux[0][j] = F_inviscid[j].density; 492c1a52365SJed Brown for (int k=0; k<3; k++) 493c1a52365SJed Brown Flux[k+1][j] = F_inviscid[j].momentum[k] - stress[k][j]; 494c1a52365SJed Brown Flux[4][j] = F_inviscid[j].E_total + Fe[j]; 495c1a52365SJed Brown } 496c1a52365SJed Brown 497c1a52365SJed Brown for (int j=0; j<3; j++) { 498c1a52365SJed Brown for (int k=0; k<5; k++) { 499*752f40e3SJed Brown Grad_v[j][k][i] = wdetJ * (dXdx[j][0] * Flux[k][0] + 500c1a52365SJed Brown dXdx[j][1] * Flux[k][1] + 501c1a52365SJed Brown dXdx[j][2] * Flux[k][2]); 502c1a52365SJed Brown } 503c1a52365SJed Brown } 504c1a52365SJed Brown 505c1a52365SJed Brown const CeedScalar body_force[5] = {0, s.U.density *g[0], s.U.density *g[1], s.U.density *g[2], 0}; 506c1a52365SJed Brown for (int j=0; j<5; j++) 507c1a52365SJed Brown v[j][i] = wdetJ * body_force[j]; 5083a8779fbSJames Wright 5093a8779fbSJames Wright // jacob_F_conv[3][5][5] = dF(convective)/dq at each direction 510c1a52365SJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 511c1a52365SJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 512c1a52365SJed Brown gamma, g, x_i); 513c1a52365SJed Brown CeedScalar grad_U[5][3]; 5143a8779fbSJames Wright for (int j=0; j<3; j++) { 515c1a52365SJed Brown grad_U[0][j] = grad_s[j].U.density; 516c1a52365SJed Brown for (int k=0; k<3; k++) grad_U[k+1][j] = grad_s[j].U.momentum[k]; 517c1a52365SJed Brown grad_U[4][j] = grad_s[j].U.E_total; 5183a8779fbSJames Wright } 5193a8779fbSJames Wright 5203a8779fbSJames Wright // strong_conv = dF/dq * dq/dx (Strong convection) 5213a8779fbSJames Wright CeedScalar strong_conv[5] = {0}; 5223a8779fbSJames Wright for (int j=0; j<3; j++) 5233a8779fbSJames Wright for (int k=0; k<5; k++) 5243a8779fbSJames Wright for (int l=0; l<5; l++) 525c1a52365SJed Brown strong_conv[k] += jacob_F_conv[j][k][l] * grad_U[l][j]; 5263a8779fbSJames Wright 527bb8a0c61SJames Wright // -- Stabilization method: none, SU, or SUPG 528bb8a0c61SJames Wright CeedScalar stab[5][3] = {{0.}}; 529bb8a0c61SJames Wright CeedScalar tau_strong_conv[5] = {0.}, tau_strong_conv_conservative[5] = {0}; 530bb8a0c61SJames Wright CeedScalar Tau_d[3] = {0.}; 5313a8779fbSJames Wright switch (context->stabilization) { 5323a8779fbSJames Wright case STAB_NONE: // Galerkin 5333a8779fbSJames Wright break; 5343a8779fbSJames Wright case STAB_SU: // SU 535c1a52365SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 536bb8a0c61SJames Wright tau_strong_conv[0] = Tau_d[0] * strong_conv[0]; 537bb8a0c61SJames Wright tau_strong_conv[1] = Tau_d[1] * strong_conv[1]; 538bb8a0c61SJames Wright tau_strong_conv[2] = Tau_d[1] * strong_conv[2]; 539bb8a0c61SJames Wright tau_strong_conv[3] = Tau_d[1] * strong_conv[3]; 540bb8a0c61SJames Wright tau_strong_conv[4] = Tau_d[2] * strong_conv[4]; 541c1a52365SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 542c1a52365SJed Brown tau_strong_conv, 543bb8a0c61SJames Wright tau_strong_conv_conservative); 5443a8779fbSJames Wright for (int j=0; j<3; j++) 5453a8779fbSJames Wright for (int k=0; k<5; k++) 5463a8779fbSJames Wright for (int l=0; l<5; l++) 547bb8a0c61SJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_conv_conservative[l]; 5483a8779fbSJames Wright 5493a8779fbSJames Wright for (int j=0; j<5; j++) 5503a8779fbSJames Wright for (int k=0; k<3; k++) 551*752f40e3SJed Brown Grad_v[k][j][i] -= wdetJ*(stab[j][0] * dXdx[k][0] + 5523a8779fbSJames Wright stab[j][1] * dXdx[k][1] + 5533a8779fbSJames Wright stab[j][2] * dXdx[k][2]); 5543a8779fbSJames Wright break; 5553a8779fbSJames Wright case STAB_SUPG: // SUPG is not implemented for explicit scheme 5563a8779fbSJames Wright break; 5573a8779fbSJames Wright } 5583a8779fbSJames Wright 5593a8779fbSJames Wright } // End Quadrature Point Loop 5603a8779fbSJames Wright 5613a8779fbSJames Wright // Return 5623a8779fbSJames Wright return 0; 5633a8779fbSJames Wright } 5643a8779fbSJames Wright 5653a8779fbSJames Wright // ***************************************************************************** 5663a8779fbSJames Wright // This QFunction implements the Navier-Stokes equations (mentioned above) with 5673a8779fbSJames Wright // implicit time stepping method 5683a8779fbSJames Wright // 5693a8779fbSJames Wright // SU = Galerkin + grad(v) . ( Ai^T * Tau * (Aj q,j) ) 5703a8779fbSJames Wright // SUPG = Galerkin + grad(v) . ( Ai^T * Tau * (q_dot + Aj q,j - body force) ) 5713a8779fbSJames Wright // (diffussive terms will be added later) 5723a8779fbSJames Wright // 5733a8779fbSJames Wright // ***************************************************************************** 5743a8779fbSJames Wright CEED_QFUNCTION(IFunction_Newtonian)(void *ctx, CeedInt Q, 5753a8779fbSJames Wright const CeedScalar *const *in, 5763a8779fbSJames Wright CeedScalar *const *out) { 5773a8779fbSJames Wright // *INDENT-OFF* 5783a8779fbSJames Wright // Inputs 5793a8779fbSJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 580*752f40e3SJed Brown (*Grad_q)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 5813a8779fbSJames Wright (*q_dot)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 5823a8779fbSJames Wright (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3], 5833a8779fbSJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[4]; 5843a8779fbSJames Wright // Outputs 5853a8779fbSJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 586*752f40e3SJed Brown (*Grad_v)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1], 587*752f40e3SJed Brown (*jac_data)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[2]; 5883a8779fbSJames Wright // *INDENT-ON* 5893a8779fbSJames Wright // Context 5903a8779fbSJames Wright NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 5913a8779fbSJames Wright const CeedScalar mu = context->mu; 5923a8779fbSJames Wright const CeedScalar cv = context->cv; 5933a8779fbSJames Wright const CeedScalar cp = context->cp; 594bb8a0c61SJames Wright const CeedScalar *g = context->g; 595bb8a0c61SJames Wright const CeedScalar dt = context->dt; 5963a8779fbSJames Wright const CeedScalar gamma = cp / cv; 597bb8a0c61SJames Wright const CeedScalar Rd = cp-cv; 5983a8779fbSJames Wright 5993a8779fbSJames Wright CeedPragmaSIMD 6003a8779fbSJames Wright // Quadrature Point Loop 6013a8779fbSJames Wright for (CeedInt i=0; i<Q; i++) { 602c1a52365SJed Brown CeedScalar U[5]; 603c1a52365SJed Brown for (int j=0; j<5; j++) U[j] = q[j][i]; 604c1a52365SJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 605c1a52365SJed Brown State s = StateFromU(context, U, x_i); 606c1a52365SJed Brown 6073a8779fbSJames Wright // -- Interp-to-Interp q_data 6083a8779fbSJames Wright const CeedScalar wdetJ = q_data[0][i]; 6093a8779fbSJames Wright // -- Interp-to-Grad q_data 6103a8779fbSJames Wright // ---- Inverse of change of coordinate matrix: X_i,j 6113a8779fbSJames Wright // *INDENT-OFF* 6123a8779fbSJames Wright const CeedScalar dXdx[3][3] = {{q_data[1][i], 6133a8779fbSJames Wright q_data[2][i], 6143a8779fbSJames Wright q_data[3][i]}, 6153a8779fbSJames Wright {q_data[4][i], 6163a8779fbSJames Wright q_data[5][i], 6173a8779fbSJames Wright q_data[6][i]}, 6183a8779fbSJames Wright {q_data[7][i], 6193a8779fbSJames Wright q_data[8][i], 6203a8779fbSJames Wright q_data[9][i]} 6213a8779fbSJames Wright }; 6223a8779fbSJames Wright // *INDENT-ON* 623c1a52365SJed Brown State grad_s[3]; 6243a8779fbSJames Wright for (int j=0; j<3; j++) { 6252f7ce6c1SJed Brown CeedScalar dx_i[3] = {0}, dU[5]; 626*752f40e3SJed Brown for (int k=0; k<5; k++) dU[k] = Grad_q[0][k][i] * dXdx[0][j] 627*752f40e3SJed Brown + Grad_q[1][k][i] * dXdx[1][j] 628*752f40e3SJed Brown + Grad_q[2][k][i] * dXdx[2][j]; 629c1a52365SJed Brown dx_i[j] = 1.; 6302f7ce6c1SJed Brown grad_s[j] = StateFromU_fwd(context, s, dU, x_i, dx_i); 6313a8779fbSJames Wright } 632c1a52365SJed Brown 633c1a52365SJed Brown CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 634c1a52365SJed Brown KMStrainRate(grad_s, strain_rate); 635c1a52365SJed Brown NewtonianStress(context, strain_rate, kmstress); 636c1a52365SJed Brown KMUnpack(kmstress, stress); 637c1a52365SJed Brown ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 638c1a52365SJed Brown 639c1a52365SJed Brown StateConservative F_inviscid[3]; 640c1a52365SJed Brown FluxInviscid(context, s, F_inviscid); 641c1a52365SJed Brown 642c1a52365SJed Brown 643c1a52365SJed Brown // Total flux 644c1a52365SJed Brown CeedScalar Flux[5][3]; 645c1a52365SJed Brown for (int j=0; j<3; j++) { 646c1a52365SJed Brown Flux[0][j] = F_inviscid[j].density; 6473a8779fbSJames Wright for (int k=0; k<3; k++) 648c1a52365SJed Brown Flux[k+1][j] = F_inviscid[j].momentum[k] - stress[k][j]; 649c1a52365SJed Brown Flux[4][j] = F_inviscid[j].E_total + Fe[j]; 650c1a52365SJed Brown } 651c1a52365SJed Brown 652c1a52365SJed Brown for (int j=0; j<3; j++) { 653c1a52365SJed Brown for (int k=0; k<5; k++) { 654*752f40e3SJed Brown Grad_v[j][k][i] = -wdetJ * (dXdx[j][0] * Flux[k][0] + 655c1a52365SJed Brown dXdx[j][1] * Flux[k][1] + 656c1a52365SJed Brown dXdx[j][2] * Flux[k][2]); 657c1a52365SJed Brown } 658c1a52365SJed Brown } 659c1a52365SJed Brown 660c1a52365SJed Brown const CeedScalar body_force[5] = {0, s.U.density *g[0], s.U.density *g[1], s.U.density *g[2], 0}; 661c1a52365SJed Brown for (int j=0; j<5; j++) 662c1a52365SJed Brown v[j][i] = wdetJ * (q_dot[j][i] - body_force[j]); 6633a8779fbSJames Wright 6643a8779fbSJames Wright // jacob_F_conv[3][5][5] = dF(convective)/dq at each direction 665c1a52365SJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 666c1a52365SJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 667c1a52365SJed Brown gamma, g, x_i); 668c1a52365SJed Brown CeedScalar grad_U[5][3]; 6693a8779fbSJames Wright for (int j=0; j<3; j++) { 670c1a52365SJed Brown grad_U[0][j] = grad_s[j].U.density; 671c1a52365SJed Brown for (int k=0; k<3; k++) grad_U[k+1][j] = grad_s[j].U.momentum[k]; 672c1a52365SJed Brown grad_U[4][j] = grad_s[j].U.E_total; 6733a8779fbSJames Wright } 674c1a52365SJed Brown 6753a8779fbSJames Wright // strong_conv = dF/dq * dq/dx (Strong convection) 6763a8779fbSJames Wright CeedScalar strong_conv[5] = {0}; 6773a8779fbSJames Wright for (int j=0; j<3; j++) 6783a8779fbSJames Wright for (int k=0; k<5; k++) 6793a8779fbSJames Wright for (int l=0; l<5; l++) 680c1a52365SJed Brown strong_conv[k] += jacob_F_conv[j][k][l] * grad_U[l][j]; 6813a8779fbSJames Wright 6823a8779fbSJames Wright // Strong residual 6833a8779fbSJames Wright CeedScalar strong_res[5]; 6843a8779fbSJames Wright for (int j=0; j<5; j++) 6853a8779fbSJames Wright strong_res[j] = q_dot[j][i] + strong_conv[j] - body_force[j]; 6863a8779fbSJames Wright 6873a8779fbSJames Wright // -- Stabilization method: none, SU, or SUPG 688bb8a0c61SJames Wright CeedScalar stab[5][3] = {{0.}}; 689bb8a0c61SJames Wright CeedScalar tau_strong_res[5] = {0.}, tau_strong_res_conservative[5] = {0}; 690bb8a0c61SJames Wright CeedScalar tau_strong_conv[5] = {0.}, tau_strong_conv_conservative[5] = {0}; 691bb8a0c61SJames Wright CeedScalar Tau_d[3] = {0.}; 6923a8779fbSJames Wright switch (context->stabilization) { 6933a8779fbSJames Wright case STAB_NONE: // Galerkin 6943a8779fbSJames Wright break; 6953a8779fbSJames Wright case STAB_SU: // SU 696c1a52365SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 697bb8a0c61SJames Wright tau_strong_conv[0] = Tau_d[0] * strong_conv[0]; 698bb8a0c61SJames Wright tau_strong_conv[1] = Tau_d[1] * strong_conv[1]; 699bb8a0c61SJames Wright tau_strong_conv[2] = Tau_d[1] * strong_conv[2]; 700bb8a0c61SJames Wright tau_strong_conv[3] = Tau_d[1] * strong_conv[3]; 701bb8a0c61SJames Wright tau_strong_conv[4] = Tau_d[2] * strong_conv[4]; 702c1a52365SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 703c1a52365SJed Brown tau_strong_conv, tau_strong_conv_conservative); 7043a8779fbSJames Wright for (int j=0; j<3; j++) 7053a8779fbSJames Wright for (int k=0; k<5; k++) 7063a8779fbSJames Wright for (int l=0; l<5; l++) 707bb8a0c61SJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_conv_conservative[l]; 7083a8779fbSJames Wright 7093a8779fbSJames Wright for (int j=0; j<5; j++) 7103a8779fbSJames Wright for (int k=0; k<3; k++) 711*752f40e3SJed Brown Grad_v[k][j][i] += wdetJ*(stab[j][0] * dXdx[k][0] + 7123a8779fbSJames Wright stab[j][1] * dXdx[k][1] + 7133a8779fbSJames Wright stab[j][2] * dXdx[k][2]); 7143a8779fbSJames Wright break; 7153a8779fbSJames Wright case STAB_SUPG: // SUPG 716c1a52365SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 717bb8a0c61SJames Wright tau_strong_res[0] = Tau_d[0] * strong_res[0]; 718bb8a0c61SJames Wright tau_strong_res[1] = Tau_d[1] * strong_res[1]; 719bb8a0c61SJames Wright tau_strong_res[2] = Tau_d[1] * strong_res[2]; 720bb8a0c61SJames Wright tau_strong_res[3] = Tau_d[1] * strong_res[3]; 721bb8a0c61SJames Wright tau_strong_res[4] = Tau_d[2] * strong_res[4]; 722bb8a0c61SJames Wright // Alternate route (useful later with primitive variable code) 723bb8a0c61SJames Wright // this function was verified against PHASTA for as IC that was as close as possible 724bb8a0c61SJames Wright // computeFluxJacobian_NSp(jacob_F_conv_p, rho, u, E, Rd, cv); 725bb8a0c61SJames Wright // it has also been verified to compute a correct through the following 726bb8a0c61SJames Wright // stab[k][j] += jacob_F_conv_p[j][k][l] * tau_strong_res[l] // flux Jacobian wrt primitive 727bb8a0c61SJames Wright // applied in the triple loop below 728bb8a0c61SJames Wright // However, it is more flops than using the existing Jacobian wrt q after q_{,Y} viz 729c1a52365SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 730c1a52365SJed Brown tau_strong_res, tau_strong_res_conservative); 7313a8779fbSJames Wright for (int j=0; j<3; j++) 7323a8779fbSJames Wright for (int k=0; k<5; k++) 7333a8779fbSJames Wright for (int l=0; l<5; l++) 734bb8a0c61SJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_res_conservative[l]; 7353a8779fbSJames Wright 7363a8779fbSJames Wright for (int j=0; j<5; j++) 7373a8779fbSJames Wright for (int k=0; k<3; k++) 738*752f40e3SJed Brown Grad_v[k][j][i] += wdetJ*(stab[j][0] * dXdx[k][0] + 7393a8779fbSJames Wright stab[j][1] * dXdx[k][1] + 7403a8779fbSJames Wright stab[j][2] * dXdx[k][2]); 7413a8779fbSJames Wright break; 7423a8779fbSJames Wright } 743*752f40e3SJed Brown for (int j=0; j<5; j++) jac_data[j][i] = U[j]; 744*752f40e3SJed Brown for (int j=0; j<3; j++) jac_data[5+j][i] = Tau_d[j]; 7453a8779fbSJames Wright 7463a8779fbSJames Wright } // End Quadrature Point Loop 7473a8779fbSJames Wright 7483a8779fbSJames Wright // Return 7493a8779fbSJames Wright return 0; 7503a8779fbSJames Wright } 7513a8779fbSJames Wright // ***************************************************************************** 7523a8779fbSJames Wright #endif // newtonian_h 753