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 23*c1a52365SJed Brown typedef struct { 24*c1a52365SJed Brown CeedScalar pressure; 25*c1a52365SJed Brown CeedScalar velocity[3]; 26*c1a52365SJed Brown CeedScalar temperature; 27*c1a52365SJed Brown } StatePrimitive; 28*c1a52365SJed Brown 29*c1a52365SJed Brown typedef struct { 30*c1a52365SJed Brown CeedScalar density; 31*c1a52365SJed Brown CeedScalar momentum[3]; 32*c1a52365SJed Brown CeedScalar E_total; 33*c1a52365SJed Brown } StateConservative; 34*c1a52365SJed Brown 35*c1a52365SJed Brown typedef struct { 36*c1a52365SJed Brown StateConservative U; 37*c1a52365SJed Brown StatePrimitive Y; 38*c1a52365SJed Brown } State; 39*c1a52365SJed Brown 40*c1a52365SJed Brown CEED_QFUNCTION_HELPER CeedScalar Dot3(const CeedScalar u[3], 41*c1a52365SJed Brown const CeedScalar v[3]) { 42*c1a52365SJed Brown return u[0]*v[0] + u[1]*v[1] + u[2]*v[2]; 43*c1a52365SJed Brown } 44*c1a52365SJed Brown 45*c1a52365SJed Brown CEED_QFUNCTION_HELPER StatePrimitive StatePrimitiveFromConservative( 46*c1a52365SJed Brown NewtonianIdealGasContext gas, StateConservative U, const CeedScalar x[3]) { 47*c1a52365SJed Brown StatePrimitive Y; 48*c1a52365SJed Brown for (int i=0; i<3; i++) Y.velocity[i] = U.momentum[i] / U.density; 49*c1a52365SJed Brown CeedScalar e_kinetic = .5 * Dot3(Y.velocity, Y.velocity); 50*c1a52365SJed Brown CeedScalar e_potential = -Dot3(gas->g, x); 51*c1a52365SJed Brown CeedScalar e_total = U.E_total / U.density; 52*c1a52365SJed Brown CeedScalar e_internal = e_total - e_kinetic - e_potential; 53*c1a52365SJed Brown Y.temperature = e_internal / gas->cv; 54*c1a52365SJed Brown Y.pressure = (gas->cp / gas->cv - 1) * U.density * e_internal; 55*c1a52365SJed Brown return Y; 56*c1a52365SJed Brown } 57*c1a52365SJed Brown 58*c1a52365SJed Brown CEED_QFUNCTION_HELPER StatePrimitive StatePrimitiveFromConservative_fwd( 59*c1a52365SJed Brown NewtonianIdealGasContext gas, State s, StateConservative dU, 60*c1a52365SJed Brown const CeedScalar x[3], const CeedScalar dx[3]) { 61*c1a52365SJed Brown StatePrimitive dY; 62*c1a52365SJed Brown for (int i=0; i<3; i++) { 63*c1a52365SJed Brown dY.velocity[i] = (dU.momentum[i] - s.Y.velocity[i] * dU.density) / s.U.density; 64*c1a52365SJed Brown } 65*c1a52365SJed Brown CeedScalar e_kinetic = .5 * Dot3(s.Y.velocity, s.Y.velocity); 66*c1a52365SJed Brown CeedScalar de_kinetic = Dot3(dY.velocity, s.Y.velocity); 67*c1a52365SJed Brown CeedScalar e_potential = -Dot3(gas->g, x); 68*c1a52365SJed Brown CeedScalar de_potential = -Dot3(gas->g, dx); 69*c1a52365SJed Brown CeedScalar e_total = s.U.E_total / s.U.density; 70*c1a52365SJed Brown CeedScalar de_total = (dU.E_total - e_total * dU.density) / s.U.density; 71*c1a52365SJed Brown CeedScalar e_internal = e_total - e_kinetic - e_potential; 72*c1a52365SJed Brown CeedScalar de_internal = de_total - de_kinetic - de_potential; 73*c1a52365SJed Brown dY.temperature = de_internal / gas->cv; 74*c1a52365SJed Brown dY.pressure = (gas->cp / gas->cv - 1) 75*c1a52365SJed Brown * (dU.density * e_internal + s.U.density * de_internal); 76*c1a52365SJed Brown return dY; 77*c1a52365SJed Brown } 78*c1a52365SJed Brown 79*c1a52365SJed Brown CEED_QFUNCTION_HELPER State StateFromU(NewtonianIdealGasContext gas, 80*c1a52365SJed Brown const CeedScalar U[5], const CeedScalar x[3]) { 81*c1a52365SJed Brown State s; 82*c1a52365SJed Brown s.U.density = U[0]; 83*c1a52365SJed Brown s.U.momentum[0] = U[1]; 84*c1a52365SJed Brown s.U.momentum[1] = U[2]; 85*c1a52365SJed Brown s.U.momentum[2] = U[3]; 86*c1a52365SJed Brown s.U.E_total = U[4]; 87*c1a52365SJed Brown s.Y = StatePrimitiveFromConservative(gas, s.U, x); 88*c1a52365SJed Brown return s; 89*c1a52365SJed Brown } 90*c1a52365SJed Brown 91*c1a52365SJed Brown CEED_QFUNCTION_HELPER void FluxInviscid(NewtonianIdealGasContext gas, State s, 92*c1a52365SJed Brown StateConservative Flux[3]) { 93*c1a52365SJed Brown for (int i=0; i<3; i++) { 94*c1a52365SJed Brown Flux[i].density = s.U.momentum[i]; 95*c1a52365SJed Brown for (int j=0; j<3; j++) 96*c1a52365SJed Brown Flux[i].momentum[j] = s.U.momentum[i] * s.Y.velocity[j] 97*c1a52365SJed Brown + s.Y.pressure * (i == j); 98*c1a52365SJed Brown Flux[i].E_total = (s.U.E_total + s.Y.pressure) * s.Y.velocity[i]; 99*c1a52365SJed Brown } 100*c1a52365SJed Brown } 101*c1a52365SJed Brown 102*c1a52365SJed Brown CEED_QFUNCTION_HELPER void FluxInviscid_fwd(NewtonianIdealGasContext gas, 103*c1a52365SJed Brown State s, State ds, StateConservative dFlux[3]) { 104*c1a52365SJed Brown for (int i=0; i<3; i++) { 105*c1a52365SJed Brown dFlux[i].density = ds.U.momentum[i]; 106*c1a52365SJed Brown for (int j=0; j<3; j++) 107*c1a52365SJed Brown dFlux[i].momentum[j] = ds.U.momentum[i] * s.Y.velocity[j] + 108*c1a52365SJed Brown s.U.momentum[i] * ds.Y.velocity[j] + ds.Y.pressure * (i == j); 109*c1a52365SJed Brown dFlux[i].E_total = (ds.U.E_total + ds.Y.pressure) * s.Y.velocity[i] + 110*c1a52365SJed Brown (s.U.E_total + s.Y.pressure) * ds.Y.velocity[i]; 111*c1a52365SJed Brown } 112*c1a52365SJed Brown } 113*c1a52365SJed Brown 114*c1a52365SJed Brown // Kelvin-Mandel notation 115*c1a52365SJed Brown CEED_QFUNCTION_HELPER void KMStrainRate(const State grad_s[3], 116*c1a52365SJed Brown CeedScalar strain_rate[6]) { 117*c1a52365SJed Brown const CeedScalar weight = 1 / sqrt(2.); 118*c1a52365SJed Brown strain_rate[0] = grad_s[0].Y.velocity[0]; 119*c1a52365SJed Brown strain_rate[1] = grad_s[1].Y.velocity[1]; 120*c1a52365SJed Brown strain_rate[2] = grad_s[2].Y.velocity[2]; 121*c1a52365SJed Brown strain_rate[3] = weight * (grad_s[2].Y.velocity[1] + grad_s[1].Y.velocity[2]); 122*c1a52365SJed Brown strain_rate[4] = weight * (grad_s[2].Y.velocity[0] + grad_s[0].Y.velocity[2]); 123*c1a52365SJed Brown strain_rate[5] = weight * (grad_s[1].Y.velocity[0] + grad_s[0].Y.velocity[1]); 124*c1a52365SJed Brown } 125*c1a52365SJed Brown 126*c1a52365SJed Brown CEED_QFUNCTION_HELPER void KMUnpack(const CeedScalar v[6], CeedScalar A[3][3]) { 127*c1a52365SJed Brown const CeedScalar weight = 1 / sqrt(2.); 128*c1a52365SJed Brown A[0][0] = v[0]; 129*c1a52365SJed Brown A[1][1] = v[1]; 130*c1a52365SJed Brown A[2][2] = v[2]; 131*c1a52365SJed Brown A[2][1] = A[1][2] = weight * v[3]; 132*c1a52365SJed Brown A[2][0] = A[0][2] = weight * v[4]; 133*c1a52365SJed Brown A[1][0] = A[0][1] = weight * v[5]; 134*c1a52365SJed Brown } 135*c1a52365SJed Brown 136*c1a52365SJed Brown CEED_QFUNCTION_HELPER void NewtonianStress(NewtonianIdealGasContext gas, 137*c1a52365SJed Brown const CeedScalar strain_rate[6], CeedScalar stress[6]) { 138*c1a52365SJed Brown CeedScalar div_u = strain_rate[0] + strain_rate[1] + strain_rate[2]; 139*c1a52365SJed Brown for (int i=0; i<6; i++) { 140*c1a52365SJed Brown stress[i] = gas->mu * (2 * strain_rate[i] + gas->lambda * div_u * (i < 3)); 141*c1a52365SJed Brown } 142*c1a52365SJed Brown } 143*c1a52365SJed Brown 144*c1a52365SJed Brown CEED_QFUNCTION_HELPER void ViscousEnergyFlux(NewtonianIdealGasContext gas, 145*c1a52365SJed Brown StatePrimitive Y, const State grad_s[3], const CeedScalar stress[3][3], 146*c1a52365SJed Brown CeedScalar Fe[3]) { 147*c1a52365SJed Brown for (int i=0; i<3; i++) { 148*c1a52365SJed Brown Fe[i] = - Y.velocity[0] * stress[0][i] 149*c1a52365SJed Brown - Y.velocity[1] * stress[1][i] 150*c1a52365SJed Brown - Y.velocity[2] * stress[2][i] 151*c1a52365SJed Brown - gas->k * grad_s[i].Y.temperature; 152*c1a52365SJed Brown } 153*c1a52365SJed Brown } 154*c1a52365SJed Brown 1553a8779fbSJames Wright // ***************************************************************************** 1563a8779fbSJames Wright // Helper function for computing flux Jacobian 1573a8779fbSJames Wright // ***************************************************************************** 1583a8779fbSJames Wright CEED_QFUNCTION_HELPER void computeFluxJacobian_NS(CeedScalar dF[3][5][5], 1593a8779fbSJames Wright const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 160bb8a0c61SJames Wright const CeedScalar gamma, const CeedScalar g[3], const CeedScalar x[3]) { 1613a8779fbSJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; // Velocity square 162bb8a0c61SJames Wright CeedScalar e_potential = -(g[0]*x[0] + g[1]*x[1] + g[2]*x[2]); 1633a8779fbSJames Wright for (CeedInt i=0; i<3; i++) { // Jacobian matrices for 3 directions 1643a8779fbSJames Wright for (CeedInt j=0; j<3; j++) { // Rows of each Jacobian matrix 165bb8a0c61SJames Wright dF[i][j+1][0] = ((i==j) ? ((gamma-1.)*(u_sq/2. - e_potential)) : 0.) - 166bb8a0c61SJames Wright u[i]*u[j]; 1673a8779fbSJames Wright for (CeedInt k=0; k<3; k++) { // Columns of each Jacobian matrix 1683a8779fbSJames Wright dF[i][0][k+1] = ((i==k) ? 1. : 0.); 1693a8779fbSJames Wright dF[i][j+1][k+1] = ((j==k) ? u[i] : 0.) + 1703a8779fbSJames Wright ((i==k) ? u[j] : 0.) - 1713a8779fbSJames Wright ((i==j) ? u[k] : 0.) * (gamma-1.); 1723a8779fbSJames Wright dF[i][4][k+1] = ((i==k) ? (E*gamma/rho - (gamma-1.)*u_sq/2.) : 0.) - 1733a8779fbSJames Wright (gamma-1.)*u[i]*u[k]; 1743a8779fbSJames Wright } 1753a8779fbSJames Wright dF[i][j+1][4] = ((i==j) ? (gamma-1.) : 0.); 1763a8779fbSJames Wright } 1773a8779fbSJames Wright dF[i][4][0] = u[i] * ((gamma-1.)*u_sq - E*gamma/rho); 1783a8779fbSJames Wright dF[i][4][4] = u[i] * gamma; 1793a8779fbSJames Wright } 1803a8779fbSJames Wright } 1813a8779fbSJames Wright 1823a8779fbSJames Wright // ***************************************************************************** 183bb8a0c61SJames Wright // Helper function for computing flux Jacobian of Primitive variables 184bb8a0c61SJames Wright // ***************************************************************************** 185bb8a0c61SJames Wright CEED_QFUNCTION_HELPER void computeFluxJacobian_NSp(CeedScalar dF[3][5][5], 186bb8a0c61SJames Wright const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 187bb8a0c61SJames Wright const CeedScalar Rd, const CeedScalar cv) { 188bb8a0c61SJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; // Velocity square 189bb8a0c61SJames Wright // TODO Add in gravity's contribution 190bb8a0c61SJames Wright 191bb8a0c61SJames Wright CeedScalar T = ( E / rho - u_sq / 2. ) / cv; 192bb8a0c61SJames Wright CeedScalar drdT = -rho / T; 193bb8a0c61SJames Wright CeedScalar drdP = 1. / ( Rd * T); 194bb8a0c61SJames Wright CeedScalar etot = E / rho ; 195bb8a0c61SJames Wright CeedScalar e2p = drdP * etot + 1. ; 196bb8a0c61SJames Wright CeedScalar e3p = ( E + rho * Rd * T ); 197bb8a0c61SJames Wright CeedScalar e4p = drdT * etot + rho * cv ; 198bb8a0c61SJames Wright 199bb8a0c61SJames Wright for (CeedInt i=0; i<3; i++) { // Jacobian matrices for 3 directions 200bb8a0c61SJames Wright for (CeedInt j=0; j<3; j++) { // j counts F^{m_j} 201bb8a0c61SJames Wright // [row][col] of A_i 202bb8a0c61SJames Wright dF[i][j+1][0] = drdP * u[i] * u[j] + ((i==j) ? 1. : 0.); // F^{{m_j} wrt p 203bb8a0c61SJames Wright for (CeedInt k=0; k<3; k++) { // k counts the wrt vel_k 2042acc7cbcSKenneth E. Jansen dF[i][0][k+1] = ((i==k) ? rho : 0.); // F^c wrt u_k 205bb8a0c61SJames Wright dF[i][j+1][k+1] = (((j==k) ? u[i] : 0.) + // F^m_j wrt u_k 206bb8a0c61SJames Wright ((i==k) ? u[j] : 0.) ) * rho; 207bb8a0c61SJames Wright dF[i][4][k+1] = rho * u[i] * u[k] 208bb8a0c61SJames Wright + ((i==k) ? e3p : 0.) ; // F^e wrt u_k 209bb8a0c61SJames Wright } 210bb8a0c61SJames Wright dF[i][j+1][4] = drdT * u[i] * u[j]; // F^{m_j} wrt T 211bb8a0c61SJames Wright } 212bb8a0c61SJames Wright dF[i][4][0] = u[i] * e2p; // F^e wrt p 213bb8a0c61SJames Wright dF[i][4][4] = u[i] * e4p; // F^e wrt T 214bb8a0c61SJames Wright dF[i][0][0] = u[i] * drdP; // F^c wrt p 215bb8a0c61SJames Wright dF[i][0][4] = u[i] * drdT; // F^c wrt T 216bb8a0c61SJames Wright } 217bb8a0c61SJames Wright } 218bb8a0c61SJames Wright 219bb8a0c61SJames Wright CEED_QFUNCTION_HELPER void PrimitiveToConservative_fwd(const CeedScalar rho, 220bb8a0c61SJames Wright const CeedScalar u[3], const CeedScalar E, const CeedScalar Rd, 221bb8a0c61SJames Wright const CeedScalar cv, const CeedScalar dY[5], CeedScalar dU[5]) { 222bb8a0c61SJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; 223bb8a0c61SJames Wright CeedScalar T = ( E / rho - u_sq / 2. ) / cv; 224bb8a0c61SJames Wright CeedScalar drdT = -rho / T; 225bb8a0c61SJames Wright CeedScalar drdP = 1. / ( Rd * T); 226bb8a0c61SJames Wright dU[0] = drdP * dY[0] + drdT * dY[4]; 227bb8a0c61SJames Wright CeedScalar de_kinetic = 0; 228bb8a0c61SJames Wright for (int i=0; i<3; i++) { 229bb8a0c61SJames Wright dU[1+i] = dU[0] * u[i] + rho * dY[1+i]; 230bb8a0c61SJames Wright de_kinetic += u[i] * dY[1+i]; 231bb8a0c61SJames Wright } 232bb8a0c61SJames Wright dU[4] = rho * cv * dY[4] + dU[0] * cv * T // internal energy: rho * e 233bb8a0c61SJames Wright + rho * de_kinetic + .5 * dU[0] * u_sq; // kinetic energy: .5 * rho * |u|^2 234bb8a0c61SJames Wright } 235bb8a0c61SJames Wright 236bb8a0c61SJames Wright // ***************************************************************************** 237bb8a0c61SJames Wright // Helper function for computing Tau elements (stabilization constant) 238bb8a0c61SJames Wright // Model from: 239bb8a0c61SJames Wright // PHASTA 240bb8a0c61SJames Wright // 241bb8a0c61SJames Wright // Tau[i] = itau=0 which is diagonal-Shakib (3 values still but not spatial) 242bb8a0c61SJames Wright // 243bb8a0c61SJames Wright // Where NOT UPDATED YET 244bb8a0c61SJames Wright // ***************************************************************************** 245bb8a0c61SJames Wright CEED_QFUNCTION_HELPER void Tau_diagPrim(CeedScalar Tau_d[3], 246bb8a0c61SJames Wright const CeedScalar dXdx[3][3], const CeedScalar u[3], 247bb8a0c61SJames Wright const CeedScalar cv, const NewtonianIdealGasContext newt_ctx, 248bb8a0c61SJames Wright const CeedScalar mu, const CeedScalar dt, 249bb8a0c61SJames Wright const CeedScalar rho) { 250bb8a0c61SJames Wright // Context 251bb8a0c61SJames Wright const CeedScalar Ctau_t = newt_ctx->Ctau_t; 252bb8a0c61SJames Wright const CeedScalar Ctau_v = newt_ctx->Ctau_v; 253bb8a0c61SJames Wright const CeedScalar Ctau_C = newt_ctx->Ctau_C; 254bb8a0c61SJames Wright const CeedScalar Ctau_M = newt_ctx->Ctau_M; 255bb8a0c61SJames Wright const CeedScalar Ctau_E = newt_ctx->Ctau_E; 256bb8a0c61SJames Wright CeedScalar gijd[6]; 257bb8a0c61SJames Wright CeedScalar tau; 258bb8a0c61SJames Wright CeedScalar dts; 259bb8a0c61SJames Wright CeedScalar fact; 260bb8a0c61SJames Wright 261bb8a0c61SJames Wright //*INDENT-OFF* 262bb8a0c61SJames Wright gijd[0] = dXdx[0][0] * dXdx[0][0] 263bb8a0c61SJames Wright + dXdx[1][0] * dXdx[1][0] 264bb8a0c61SJames Wright + dXdx[2][0] * dXdx[2][0]; 265bb8a0c61SJames Wright 266bb8a0c61SJames Wright gijd[1] = dXdx[0][0] * dXdx[0][1] 267bb8a0c61SJames Wright + dXdx[1][0] * dXdx[1][1] 268bb8a0c61SJames Wright + dXdx[2][0] * dXdx[2][1]; 269bb8a0c61SJames Wright 270bb8a0c61SJames Wright gijd[2] = dXdx[0][1] * dXdx[0][1] 271bb8a0c61SJames Wright + dXdx[1][1] * dXdx[1][1] 272bb8a0c61SJames Wright + dXdx[2][1] * dXdx[2][1]; 273bb8a0c61SJames Wright 274bb8a0c61SJames Wright gijd[3] = dXdx[0][0] * dXdx[0][2] 275bb8a0c61SJames Wright + dXdx[1][0] * dXdx[1][2] 276bb8a0c61SJames Wright + dXdx[2][0] * dXdx[2][2]; 277bb8a0c61SJames Wright 278bb8a0c61SJames Wright gijd[4] = dXdx[0][1] * dXdx[0][2] 279bb8a0c61SJames Wright + dXdx[1][1] * dXdx[1][2] 280bb8a0c61SJames Wright + dXdx[2][1] * dXdx[2][2]; 281bb8a0c61SJames Wright 282bb8a0c61SJames Wright gijd[5] = dXdx[0][2] * dXdx[0][2] 283bb8a0c61SJames Wright + dXdx[1][2] * dXdx[1][2] 284bb8a0c61SJames Wright + dXdx[2][2] * dXdx[2][2]; 285bb8a0c61SJames Wright //*INDENT-ON* 286bb8a0c61SJames Wright 287bb8a0c61SJames Wright dts = Ctau_t / dt ; 288bb8a0c61SJames Wright 289bb8a0c61SJames Wright tau = rho*rho*((4. * dts * dts) 290bb8a0c61SJames Wright + u[0] * ( u[0] * gijd[0] + 2. * ( u[1] * gijd[1] + u[2] * gijd[3])) 291bb8a0c61SJames Wright + u[1] * ( u[1] * gijd[2] + 2. * u[2] * gijd[4]) 292bb8a0c61SJames Wright + u[2] * u[2] * gijd[5]) 293bb8a0c61SJames Wright + Ctau_v* mu * mu * 294bb8a0c61SJames Wright (gijd[0]*gijd[0] + gijd[2]*gijd[2] + gijd[5]*gijd[5] + 295bb8a0c61SJames Wright + 2. * (gijd[1]*gijd[1] + gijd[3]*gijd[3] + gijd[4]*gijd[4])); 296bb8a0c61SJames Wright 297bb8a0c61SJames Wright fact=sqrt(tau); 298bb8a0c61SJames Wright 299bb8a0c61SJames Wright Tau_d[0] = Ctau_C * fact / (rho*(gijd[0] + gijd[2] + gijd[5]))*0.125; 300bb8a0c61SJames Wright 301bb8a0c61SJames Wright Tau_d[1] = Ctau_M / fact; 302bb8a0c61SJames Wright Tau_d[2] = Ctau_E / ( fact * cv ); 303bb8a0c61SJames Wright 304bb8a0c61SJames Wright // consider putting back the way I initially had it Ctau_E * Tau_d[1] /cv 305bb8a0c61SJames Wright // to avoid a division if the compiler is smart enough to see that cv IS 306bb8a0c61SJames Wright // a constant that it could invert once for all elements 307bb8a0c61SJames Wright // but in that case energy tau is scaled by the product of Ctau_E * Ctau_M 308bb8a0c61SJames Wright // OR we could absorb cv into Ctau_E but this puts more burden on user to 309bb8a0c61SJames Wright // know how to change constants with a change of fluid or units. Same for 310bb8a0c61SJames Wright // Ctau_v * mu * mu IF AND ONLY IF we don't add viscosity law =f(T) 311bb8a0c61SJames Wright } 312bb8a0c61SJames Wright 313bb8a0c61SJames Wright // ***************************************************************************** 3143a8779fbSJames Wright // This QFunction sets a "still" initial condition for generic Newtonian IG problems 3153a8779fbSJames Wright // ***************************************************************************** 3163a8779fbSJames Wright CEED_QFUNCTION(ICsNewtonianIG)(void *ctx, CeedInt Q, 3173a8779fbSJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 3183a8779fbSJames Wright // Inputs 3193a8779fbSJames Wright const CeedScalar (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 3203a8779fbSJames Wright 3213a8779fbSJames Wright // Outputs 3223a8779fbSJames Wright CeedScalar (*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 3233a8779fbSJames Wright 324bb8a0c61SJames Wright // Context 325bb8a0c61SJames Wright const SetupContext context = (SetupContext)ctx; 326bb8a0c61SJames Wright const CeedScalar theta0 = context->theta0; 327bb8a0c61SJames Wright const CeedScalar P0 = context->P0; 328bb8a0c61SJames Wright const CeedScalar cv = context->cv; 329bb8a0c61SJames Wright const CeedScalar cp = context->cp; 330bb8a0c61SJames Wright const CeedScalar *g = context->g; 331bb8a0c61SJames Wright const CeedScalar Rd = cp - cv; 332bb8a0c61SJames Wright 3333a8779fbSJames Wright // Quadrature Point Loop 3343a8779fbSJames Wright CeedPragmaSIMD 3353a8779fbSJames Wright for (CeedInt i=0; i<Q; i++) { 3363a8779fbSJames Wright CeedScalar q[5] = {0.}; 3373a8779fbSJames Wright 3383a8779fbSJames Wright // Setup 3393a8779fbSJames Wright // -- Coordinates 340bb8a0c61SJames Wright const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 341bb8a0c61SJames Wright const CeedScalar e_potential = -(g[0]*x[0] + g[1]*x[1] + g[2]*x[2]); 3423a8779fbSJames Wright 3433a8779fbSJames Wright // -- Density 344bb8a0c61SJames Wright const CeedScalar rho = P0 / (Rd*theta0); 3453a8779fbSJames Wright 3463a8779fbSJames Wright // Initial Conditions 3473a8779fbSJames Wright q[0] = rho; 3483a8779fbSJames Wright q[1] = 0.0; 3493a8779fbSJames Wright q[2] = 0.0; 3503a8779fbSJames Wright q[3] = 0.0; 351bb8a0c61SJames Wright q[4] = rho * (cv*theta0 + e_potential); 3523a8779fbSJames Wright 3533a8779fbSJames Wright for (CeedInt j=0; j<5; j++) 3543a8779fbSJames Wright q0[j][i] = q[j]; 3553a8779fbSJames Wright } // End of Quadrature Point Loop 3563a8779fbSJames Wright return 0; 3573a8779fbSJames Wright } 3583a8779fbSJames Wright 3593a8779fbSJames Wright // ***************************************************************************** 3603a8779fbSJames Wright // This QFunction implements the following formulation of Navier-Stokes with 3613a8779fbSJames Wright // explicit time stepping method 3623a8779fbSJames Wright // 3633a8779fbSJames Wright // This is 3D compressible Navier-Stokes in conservation form with state 3643a8779fbSJames Wright // variables of density, momentum density, and total energy density. 3653a8779fbSJames Wright // 3663a8779fbSJames Wright // State Variables: q = ( rho, U1, U2, U3, E ) 3673a8779fbSJames Wright // rho - Mass Density 3683a8779fbSJames Wright // Ui - Momentum Density, Ui = rho ui 3693a8779fbSJames Wright // E - Total Energy Density, E = rho (cv T + (u u)/2 + g z) 3703a8779fbSJames Wright // 3713a8779fbSJames Wright // Navier-Stokes Equations: 3723a8779fbSJames Wright // drho/dt + div( U ) = 0 3733a8779fbSJames Wright // dU/dt + div( rho (u x u) + P I3 ) + rho g khat = div( Fu ) 3743a8779fbSJames Wright // dE/dt + div( (E + P) u ) = div( Fe ) 3753a8779fbSJames Wright // 3763a8779fbSJames Wright // Viscous Stress: 3773a8779fbSJames Wright // Fu = mu (grad( u ) + grad( u )^T + lambda div ( u ) I3) 3783a8779fbSJames Wright // 3793a8779fbSJames Wright // Thermal Stress: 3803a8779fbSJames Wright // Fe = u Fu + k grad( T ) 381bb8a0c61SJames Wright // Equation of State 3823a8779fbSJames Wright // P = (gamma - 1) (E - rho (u u) / 2 - rho g z) 3833a8779fbSJames Wright // 3843a8779fbSJames Wright // Stabilization: 3853a8779fbSJames Wright // Tau = diag(TauC, TauM, TauM, TauM, TauE) 3863a8779fbSJames Wright // f1 = rho sqrt(ui uj gij) 3873a8779fbSJames Wright // gij = dXi/dX * dXi/dX 3883a8779fbSJames Wright // TauC = Cc f1 / (8 gii) 3893a8779fbSJames Wright // TauM = min( 1 , 1 / f1 ) 3903a8779fbSJames Wright // TauE = TauM / (Ce cv) 3913a8779fbSJames Wright // 3923a8779fbSJames Wright // SU = Galerkin + grad(v) . ( Ai^T * Tau * (Aj q,j) ) 3933a8779fbSJames Wright // 3943a8779fbSJames Wright // Constants: 3953a8779fbSJames Wright // lambda = - 2 / 3, From Stokes hypothesis 3963a8779fbSJames Wright // mu , Dynamic viscosity 3973a8779fbSJames Wright // k , Thermal conductivity 3983a8779fbSJames Wright // cv , Specific heat, constant volume 3993a8779fbSJames Wright // cp , Specific heat, constant pressure 4003a8779fbSJames Wright // g , Gravity 4013a8779fbSJames Wright // gamma = cp / cv, Specific heat ratio 4023a8779fbSJames Wright // 4033a8779fbSJames Wright // We require the product of the inverse of the Jacobian (dXdx_j,k) and 4043a8779fbSJames Wright // its transpose (dXdx_k,j) to properly compute integrals of the form: 4053a8779fbSJames Wright // int( gradv gradu ) 4063a8779fbSJames Wright // 4073a8779fbSJames Wright // ***************************************************************************** 408*c1a52365SJed Brown CEED_QFUNCTION(RHSFunction_Newtonian)(void *ctx, CeedInt Q, 4093a8779fbSJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 4103a8779fbSJames Wright // *INDENT-OFF* 4113a8779fbSJames Wright // Inputs 4123a8779fbSJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 4133a8779fbSJames Wright (*dq)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 4143a8779fbSJames Wright (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 4153a8779fbSJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 4163a8779fbSJames Wright // Outputs 4173a8779fbSJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 4183a8779fbSJames Wright (*dv)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1]; 4193a8779fbSJames Wright // *INDENT-ON* 4203a8779fbSJames Wright 4213a8779fbSJames Wright // Context 4223a8779fbSJames Wright NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 4233a8779fbSJames Wright const CeedScalar mu = context->mu; 4243a8779fbSJames Wright const CeedScalar cv = context->cv; 4253a8779fbSJames Wright const CeedScalar cp = context->cp; 426bb8a0c61SJames Wright const CeedScalar *g = context->g; 427bb8a0c61SJames Wright const CeedScalar dt = context->dt; 4283a8779fbSJames Wright const CeedScalar gamma = cp / cv; 429bb8a0c61SJames Wright const CeedScalar Rd = cp - cv; 4303a8779fbSJames Wright 4313a8779fbSJames Wright CeedPragmaSIMD 4323a8779fbSJames Wright // Quadrature Point Loop 4333a8779fbSJames Wright for (CeedInt i=0; i<Q; i++) { 434*c1a52365SJed Brown CeedScalar U[5]; 435*c1a52365SJed Brown for (int j=0; j<5; j++) U[j] = q[j][i]; 436*c1a52365SJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 437*c1a52365SJed Brown State s = StateFromU(context, U, x_i); 438*c1a52365SJed Brown 4393a8779fbSJames Wright // -- Interp-to-Interp q_data 4403a8779fbSJames Wright const CeedScalar wdetJ = q_data[0][i]; 4413a8779fbSJames Wright // -- Interp-to-Grad q_data 4423a8779fbSJames Wright // ---- Inverse of change of coordinate matrix: X_i,j 4433a8779fbSJames Wright // *INDENT-OFF* 4443a8779fbSJames Wright const CeedScalar dXdx[3][3] = {{q_data[1][i], 4453a8779fbSJames Wright q_data[2][i], 4463a8779fbSJames Wright q_data[3][i]}, 4473a8779fbSJames Wright {q_data[4][i], 4483a8779fbSJames Wright q_data[5][i], 4493a8779fbSJames Wright q_data[6][i]}, 4503a8779fbSJames Wright {q_data[7][i], 4513a8779fbSJames Wright q_data[8][i], 4523a8779fbSJames Wright q_data[9][i]} 4533a8779fbSJames Wright }; 4543a8779fbSJames Wright // *INDENT-ON* 4553a8779fbSJames Wright 456*c1a52365SJed Brown State grad_s[3]; 457*c1a52365SJed Brown for (int j=0; j<3; j++) { 458*c1a52365SJed Brown CeedScalar dx_i[3] = {0}; 459*c1a52365SJed Brown grad_s[j].U.density = dq[0][0][i] * dXdx[0][j] 460*c1a52365SJed Brown + dq[1][0][i] * dXdx[1][j] + dq[2][0][i] * dXdx[2][j]; 461*c1a52365SJed Brown for (int k=0; k<3; k++) grad_s[j].U.momentum[k] = dq[0][k+1][i] * dXdx[0][j] 462*c1a52365SJed Brown + dq[1][k+1][i] * dXdx[1][j] + dq[2][k+1][i] * dXdx[2][j]; 463*c1a52365SJed Brown grad_s[j].U.E_total = dq[0][4][i] * dXdx[0][j] + dq[1][4][i] * dXdx[1][j] + 464*c1a52365SJed Brown dq[2][4][i] * dXdx[2][j]; 465*c1a52365SJed Brown dx_i[j] = 1.; 466*c1a52365SJed Brown grad_s[j].Y = StatePrimitiveFromConservative_fwd(context, s, grad_s[j].U, 467*c1a52365SJed Brown x_i, dx_i); 468*c1a52365SJed Brown } 469*c1a52365SJed Brown 470*c1a52365SJed Brown CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 471*c1a52365SJed Brown KMStrainRate(grad_s, strain_rate); 472*c1a52365SJed Brown NewtonianStress(context, strain_rate, kmstress); 473*c1a52365SJed Brown KMUnpack(kmstress, stress); 474*c1a52365SJed Brown ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 475*c1a52365SJed Brown 476*c1a52365SJed Brown StateConservative F_inviscid[3]; 477*c1a52365SJed Brown FluxInviscid(context, s, F_inviscid); 478*c1a52365SJed Brown 479*c1a52365SJed Brown // Total flux 480*c1a52365SJed Brown CeedScalar Flux[5][3]; 481*c1a52365SJed Brown for (int j=0; j<3; j++) { 482*c1a52365SJed Brown Flux[0][j] = F_inviscid[j].density; 483*c1a52365SJed Brown for (int k=0; k<3; k++) 484*c1a52365SJed Brown Flux[k+1][j] = F_inviscid[j].momentum[k] - stress[k][j]; 485*c1a52365SJed Brown Flux[4][j] = F_inviscid[j].E_total + Fe[j]; 486*c1a52365SJed Brown } 487*c1a52365SJed Brown 488*c1a52365SJed Brown for (int j=0; j<3; j++) { 489*c1a52365SJed Brown for (int k=0; k<5; k++) { 490*c1a52365SJed Brown dv[j][k][i] = wdetJ * (dXdx[j][0] * Flux[k][0] + 491*c1a52365SJed Brown dXdx[j][1] * Flux[k][1] + 492*c1a52365SJed Brown dXdx[j][2] * Flux[k][2]); 493*c1a52365SJed Brown } 494*c1a52365SJed Brown } 495*c1a52365SJed Brown 496*c1a52365SJed Brown const CeedScalar body_force[5] = {0, s.U.density *g[0], s.U.density *g[1], s.U.density *g[2], 0}; 497*c1a52365SJed Brown for (int j=0; j<5; j++) 498*c1a52365SJed Brown v[j][i] = wdetJ * body_force[j]; 4993a8779fbSJames Wright 5003a8779fbSJames Wright // jacob_F_conv[3][5][5] = dF(convective)/dq at each direction 501*c1a52365SJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 502*c1a52365SJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 503*c1a52365SJed Brown gamma, g, x_i); 504*c1a52365SJed Brown CeedScalar grad_U[5][3]; 5053a8779fbSJames Wright for (int j=0; j<3; j++) { 506*c1a52365SJed Brown grad_U[0][j] = grad_s[j].U.density; 507*c1a52365SJed Brown for (int k=0; k<3; k++) grad_U[k+1][j] = grad_s[j].U.momentum[k]; 508*c1a52365SJed Brown grad_U[4][j] = grad_s[j].U.E_total; 5093a8779fbSJames Wright } 5103a8779fbSJames Wright 5113a8779fbSJames Wright // strong_conv = dF/dq * dq/dx (Strong convection) 5123a8779fbSJames Wright CeedScalar strong_conv[5] = {0}; 5133a8779fbSJames Wright for (int j=0; j<3; j++) 5143a8779fbSJames Wright for (int k=0; k<5; k++) 5153a8779fbSJames Wright for (int l=0; l<5; l++) 516*c1a52365SJed Brown strong_conv[k] += jacob_F_conv[j][k][l] * grad_U[l][j]; 5173a8779fbSJames Wright 518bb8a0c61SJames Wright // -- Stabilization method: none, SU, or SUPG 519bb8a0c61SJames Wright CeedScalar stab[5][3] = {{0.}}; 520bb8a0c61SJames Wright CeedScalar tau_strong_conv[5] = {0.}, tau_strong_conv_conservative[5] = {0}; 521bb8a0c61SJames Wright CeedScalar Tau_d[3] = {0.}; 5223a8779fbSJames Wright switch (context->stabilization) { 5233a8779fbSJames Wright case STAB_NONE: // Galerkin 5243a8779fbSJames Wright break; 5253a8779fbSJames Wright case STAB_SU: // SU 526*c1a52365SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 527bb8a0c61SJames Wright tau_strong_conv[0] = Tau_d[0] * strong_conv[0]; 528bb8a0c61SJames Wright tau_strong_conv[1] = Tau_d[1] * strong_conv[1]; 529bb8a0c61SJames Wright tau_strong_conv[2] = Tau_d[1] * strong_conv[2]; 530bb8a0c61SJames Wright tau_strong_conv[3] = Tau_d[1] * strong_conv[3]; 531bb8a0c61SJames Wright tau_strong_conv[4] = Tau_d[2] * strong_conv[4]; 532*c1a52365SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 533*c1a52365SJed Brown tau_strong_conv, 534bb8a0c61SJames Wright tau_strong_conv_conservative); 5353a8779fbSJames Wright for (int j=0; j<3; j++) 5363a8779fbSJames Wright for (int k=0; k<5; k++) 5373a8779fbSJames Wright for (int l=0; l<5; l++) 538bb8a0c61SJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_conv_conservative[l]; 5393a8779fbSJames Wright 5403a8779fbSJames Wright for (int j=0; j<5; j++) 5413a8779fbSJames Wright for (int k=0; k<3; k++) 5423a8779fbSJames Wright dv[k][j][i] -= wdetJ*(stab[j][0] * dXdx[k][0] + 5433a8779fbSJames Wright stab[j][1] * dXdx[k][1] + 5443a8779fbSJames Wright stab[j][2] * dXdx[k][2]); 5453a8779fbSJames Wright break; 5463a8779fbSJames Wright case STAB_SUPG: // SUPG is not implemented for explicit scheme 5473a8779fbSJames Wright break; 5483a8779fbSJames Wright } 5493a8779fbSJames Wright 5503a8779fbSJames Wright } // End Quadrature Point Loop 5513a8779fbSJames Wright 5523a8779fbSJames Wright // Return 5533a8779fbSJames Wright return 0; 5543a8779fbSJames Wright } 5553a8779fbSJames Wright 5563a8779fbSJames Wright // ***************************************************************************** 5573a8779fbSJames Wright // This QFunction implements the Navier-Stokes equations (mentioned above) with 5583a8779fbSJames Wright // implicit time stepping method 5593a8779fbSJames Wright // 5603a8779fbSJames Wright // SU = Galerkin + grad(v) . ( Ai^T * Tau * (Aj q,j) ) 5613a8779fbSJames Wright // SUPG = Galerkin + grad(v) . ( Ai^T * Tau * (q_dot + Aj q,j - body force) ) 5623a8779fbSJames Wright // (diffussive terms will be added later) 5633a8779fbSJames Wright // 5643a8779fbSJames Wright // ***************************************************************************** 5653a8779fbSJames Wright CEED_QFUNCTION(IFunction_Newtonian)(void *ctx, CeedInt Q, 5663a8779fbSJames Wright const CeedScalar *const *in, 5673a8779fbSJames Wright CeedScalar *const *out) { 5683a8779fbSJames Wright // *INDENT-OFF* 5693a8779fbSJames Wright // Inputs 5703a8779fbSJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 5713a8779fbSJames Wright (*dq)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 5723a8779fbSJames Wright (*q_dot)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 5733a8779fbSJames Wright (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3], 5743a8779fbSJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[4]; 5753a8779fbSJames Wright // Outputs 5763a8779fbSJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 5773a8779fbSJames Wright (*dv)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1]; 5783a8779fbSJames Wright // *INDENT-ON* 5793a8779fbSJames Wright // Context 5803a8779fbSJames Wright NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 5813a8779fbSJames Wright const CeedScalar mu = context->mu; 5823a8779fbSJames Wright const CeedScalar cv = context->cv; 5833a8779fbSJames Wright const CeedScalar cp = context->cp; 584bb8a0c61SJames Wright const CeedScalar *g = context->g; 585bb8a0c61SJames Wright const CeedScalar dt = context->dt; 5863a8779fbSJames Wright const CeedScalar gamma = cp / cv; 587bb8a0c61SJames Wright const CeedScalar Rd = cp-cv; 5883a8779fbSJames Wright 5893a8779fbSJames Wright CeedPragmaSIMD 5903a8779fbSJames Wright // Quadrature Point Loop 5913a8779fbSJames Wright for (CeedInt i=0; i<Q; i++) { 592*c1a52365SJed Brown CeedScalar U[5]; 593*c1a52365SJed Brown for (int j=0; j<5; j++) U[j] = q[j][i]; 594*c1a52365SJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 595*c1a52365SJed Brown State s = StateFromU(context, U, x_i); 596*c1a52365SJed Brown 5973a8779fbSJames Wright // -- Interp-to-Interp q_data 5983a8779fbSJames Wright const CeedScalar wdetJ = q_data[0][i]; 5993a8779fbSJames Wright // -- Interp-to-Grad q_data 6003a8779fbSJames Wright // ---- Inverse of change of coordinate matrix: X_i,j 6013a8779fbSJames Wright // *INDENT-OFF* 6023a8779fbSJames Wright const CeedScalar dXdx[3][3] = {{q_data[1][i], 6033a8779fbSJames Wright q_data[2][i], 6043a8779fbSJames Wright q_data[3][i]}, 6053a8779fbSJames Wright {q_data[4][i], 6063a8779fbSJames Wright q_data[5][i], 6073a8779fbSJames Wright q_data[6][i]}, 6083a8779fbSJames Wright {q_data[7][i], 6093a8779fbSJames Wright q_data[8][i], 6103a8779fbSJames Wright q_data[9][i]} 6113a8779fbSJames Wright }; 6123a8779fbSJames Wright // *INDENT-ON* 613*c1a52365SJed Brown State grad_s[3]; 6143a8779fbSJames Wright for (int j=0; j<3; j++) { 615*c1a52365SJed Brown CeedScalar dx_i[3]; 616*c1a52365SJed Brown grad_s[j].U.density = dq[0][0][i] * dXdx[0][j] 617*c1a52365SJed Brown + dq[1][0][i] * dXdx[1][j] + dq[2][0][i] * dXdx[2][j]; 618*c1a52365SJed Brown for (int k=0; k<3; k++) grad_s[j].U.momentum[k] = dq[0][k+1][i] * dXdx[0][j] 619*c1a52365SJed Brown + dq[1][k+1][i] * dXdx[1][j] + dq[2][k+1][i] * dXdx[2][j]; 620*c1a52365SJed Brown grad_s[j].U.E_total = dq[0][4][i] * dXdx[0][j] + dq[1][4][i] * dXdx[1][j] + 621*c1a52365SJed Brown dq[2][4][i] * dXdx[2][j]; 622*c1a52365SJed Brown dx_i[j] = 1.; 623*c1a52365SJed Brown grad_s[j].Y = StatePrimitiveFromConservative_fwd(context, s, grad_s[j].U, 624*c1a52365SJed Brown x_i, dx_i); 6253a8779fbSJames Wright } 626*c1a52365SJed Brown 627*c1a52365SJed Brown CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 628*c1a52365SJed Brown KMStrainRate(grad_s, strain_rate); 629*c1a52365SJed Brown NewtonianStress(context, strain_rate, kmstress); 630*c1a52365SJed Brown KMUnpack(kmstress, stress); 631*c1a52365SJed Brown ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 632*c1a52365SJed Brown 633*c1a52365SJed Brown StateConservative F_inviscid[3]; 634*c1a52365SJed Brown FluxInviscid(context, s, F_inviscid); 635*c1a52365SJed Brown 636*c1a52365SJed Brown 637*c1a52365SJed Brown // Total flux 638*c1a52365SJed Brown CeedScalar Flux[5][3]; 639*c1a52365SJed Brown for (int j=0; j<3; j++) { 640*c1a52365SJed Brown Flux[0][j] = F_inviscid[j].density; 6413a8779fbSJames Wright for (int k=0; k<3; k++) 642*c1a52365SJed Brown Flux[k+1][j] = F_inviscid[j].momentum[k] - stress[k][j]; 643*c1a52365SJed Brown Flux[4][j] = F_inviscid[j].E_total + Fe[j]; 644*c1a52365SJed Brown } 645*c1a52365SJed Brown 646*c1a52365SJed Brown for (int j=0; j<3; j++) { 647*c1a52365SJed Brown for (int k=0; k<5; k++) { 648*c1a52365SJed Brown dv[j][k][i] = -wdetJ * (dXdx[j][0] * Flux[k][0] + 649*c1a52365SJed Brown dXdx[j][1] * Flux[k][1] + 650*c1a52365SJed Brown dXdx[j][2] * Flux[k][2]); 651*c1a52365SJed Brown } 652*c1a52365SJed Brown } 653*c1a52365SJed Brown 654*c1a52365SJed Brown const CeedScalar body_force[5] = {0, s.U.density *g[0], s.U.density *g[1], s.U.density *g[2], 0}; 655*c1a52365SJed Brown for (int j=0; j<5; j++) 656*c1a52365SJed Brown v[j][i] = wdetJ * (q_dot[j][i] - body_force[j]); 6573a8779fbSJames Wright 6583a8779fbSJames Wright // jacob_F_conv[3][5][5] = dF(convective)/dq at each direction 659*c1a52365SJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 660*c1a52365SJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 661*c1a52365SJed Brown gamma, g, x_i); 662*c1a52365SJed Brown CeedScalar grad_U[5][3]; 6633a8779fbSJames Wright for (int j=0; j<3; j++) { 664*c1a52365SJed Brown grad_U[0][j] = grad_s[j].U.density; 665*c1a52365SJed Brown for (int k=0; k<3; k++) grad_U[k+1][j] = grad_s[j].U.momentum[k]; 666*c1a52365SJed Brown grad_U[4][j] = grad_s[j].U.E_total; 6673a8779fbSJames Wright } 668*c1a52365SJed Brown 6693a8779fbSJames Wright // strong_conv = dF/dq * dq/dx (Strong convection) 6703a8779fbSJames Wright CeedScalar strong_conv[5] = {0}; 6713a8779fbSJames Wright for (int j=0; j<3; j++) 6723a8779fbSJames Wright for (int k=0; k<5; k++) 6733a8779fbSJames Wright for (int l=0; l<5; l++) 674*c1a52365SJed Brown strong_conv[k] += jacob_F_conv[j][k][l] * grad_U[l][j]; 6753a8779fbSJames Wright 6763a8779fbSJames Wright // Strong residual 6773a8779fbSJames Wright CeedScalar strong_res[5]; 6783a8779fbSJames Wright for (int j=0; j<5; j++) 6793a8779fbSJames Wright strong_res[j] = q_dot[j][i] + strong_conv[j] - body_force[j]; 6803a8779fbSJames Wright 6813a8779fbSJames Wright // -- Stabilization method: none, SU, or SUPG 682bb8a0c61SJames Wright CeedScalar stab[5][3] = {{0.}}; 683bb8a0c61SJames Wright CeedScalar tau_strong_res[5] = {0.}, tau_strong_res_conservative[5] = {0}; 684bb8a0c61SJames Wright CeedScalar tau_strong_conv[5] = {0.}, tau_strong_conv_conservative[5] = {0}; 685bb8a0c61SJames Wright CeedScalar Tau_d[3] = {0.}; 6863a8779fbSJames Wright switch (context->stabilization) { 6873a8779fbSJames Wright case STAB_NONE: // Galerkin 6883a8779fbSJames Wright break; 6893a8779fbSJames Wright case STAB_SU: // SU 690*c1a52365SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 691bb8a0c61SJames Wright tau_strong_conv[0] = Tau_d[0] * strong_conv[0]; 692bb8a0c61SJames Wright tau_strong_conv[1] = Tau_d[1] * strong_conv[1]; 693bb8a0c61SJames Wright tau_strong_conv[2] = Tau_d[1] * strong_conv[2]; 694bb8a0c61SJames Wright tau_strong_conv[3] = Tau_d[1] * strong_conv[3]; 695bb8a0c61SJames Wright tau_strong_conv[4] = Tau_d[2] * strong_conv[4]; 696*c1a52365SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 697*c1a52365SJed Brown tau_strong_conv, tau_strong_conv_conservative); 6983a8779fbSJames Wright for (int j=0; j<3; j++) 6993a8779fbSJames Wright for (int k=0; k<5; k++) 7003a8779fbSJames Wright for (int l=0; l<5; l++) 701bb8a0c61SJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_conv_conservative[l]; 7023a8779fbSJames Wright 7033a8779fbSJames Wright for (int j=0; j<5; j++) 7043a8779fbSJames Wright for (int k=0; k<3; k++) 7053a8779fbSJames Wright dv[k][j][i] += wdetJ*(stab[j][0] * dXdx[k][0] + 7063a8779fbSJames Wright stab[j][1] * dXdx[k][1] + 7073a8779fbSJames Wright stab[j][2] * dXdx[k][2]); 7083a8779fbSJames Wright break; 7093a8779fbSJames Wright case STAB_SUPG: // SUPG 710*c1a52365SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 711bb8a0c61SJames Wright tau_strong_res[0] = Tau_d[0] * strong_res[0]; 712bb8a0c61SJames Wright tau_strong_res[1] = Tau_d[1] * strong_res[1]; 713bb8a0c61SJames Wright tau_strong_res[2] = Tau_d[1] * strong_res[2]; 714bb8a0c61SJames Wright tau_strong_res[3] = Tau_d[1] * strong_res[3]; 715bb8a0c61SJames Wright tau_strong_res[4] = Tau_d[2] * strong_res[4]; 716bb8a0c61SJames Wright // Alternate route (useful later with primitive variable code) 717bb8a0c61SJames Wright // this function was verified against PHASTA for as IC that was as close as possible 718bb8a0c61SJames Wright // computeFluxJacobian_NSp(jacob_F_conv_p, rho, u, E, Rd, cv); 719bb8a0c61SJames Wright // it has also been verified to compute a correct through the following 720bb8a0c61SJames Wright // stab[k][j] += jacob_F_conv_p[j][k][l] * tau_strong_res[l] // flux Jacobian wrt primitive 721bb8a0c61SJames Wright // applied in the triple loop below 722bb8a0c61SJames Wright // However, it is more flops than using the existing Jacobian wrt q after q_{,Y} viz 723*c1a52365SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 724*c1a52365SJed Brown tau_strong_res, tau_strong_res_conservative); 7253a8779fbSJames Wright for (int j=0; j<3; j++) 7263a8779fbSJames Wright for (int k=0; k<5; k++) 7273a8779fbSJames Wright for (int l=0; l<5; l++) 728bb8a0c61SJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_res_conservative[l]; 7293a8779fbSJames Wright 7303a8779fbSJames Wright for (int j=0; j<5; j++) 7313a8779fbSJames Wright for (int k=0; k<3; k++) 7323a8779fbSJames Wright dv[k][j][i] += wdetJ*(stab[j][0] * dXdx[k][0] + 7333a8779fbSJames Wright stab[j][1] * dXdx[k][1] + 7343a8779fbSJames Wright stab[j][2] * dXdx[k][2]); 7353a8779fbSJames Wright break; 7363a8779fbSJames Wright } 7373a8779fbSJames Wright 7383a8779fbSJames Wright } // End Quadrature Point Loop 7393a8779fbSJames Wright 7403a8779fbSJames Wright // Return 7413a8779fbSJames Wright return 0; 7423a8779fbSJames Wright } 7433a8779fbSJames Wright // ***************************************************************************** 7443a8779fbSJames Wright #endif // newtonian_h 745