13d8e8822SJeremy L Thompson // Copyright (c) 2017-2022, Lawrence Livermore National Security, LLC and other CEED contributors. 23d8e8822SJeremy L Thompson // All Rights Reserved. See the top-level LICENSE and NOTICE files for details. 388b783a1SJames Wright // 43d8e8822SJeremy L Thompson // SPDX-License-Identifier: BSD-2-Clause 588b783a1SJames Wright // 63d8e8822SJeremy L Thompson // This file is part of CEED: http://github.com/ceed 788b783a1SJames Wright 888b783a1SJames Wright /// @file 988b783a1SJames Wright /// Operator for Navier-Stokes example using PETSc 1088b783a1SJames Wright 1188b783a1SJames Wright 1288b783a1SJames Wright #ifndef newtonian_h 1388b783a1SJames Wright #define newtonian_h 1488b783a1SJames Wright 1588b783a1SJames Wright #include <math.h> 1688b783a1SJames Wright #include <ceed.h> 17841e4c73SJed Brown #include "newtonian_types.h" 1888b783a1SJames Wright 1988b783a1SJames Wright #ifndef M_PI 2088b783a1SJames Wright #define M_PI 3.14159265358979323846 2188b783a1SJames Wright #endif 2288b783a1SJames Wright 235c677226SJed Brown typedef struct { 245c677226SJed Brown CeedScalar pressure; 255c677226SJed Brown CeedScalar velocity[3]; 265c677226SJed Brown CeedScalar temperature; 275c677226SJed Brown } StatePrimitive; 285c677226SJed Brown 295c677226SJed Brown typedef struct { 305c677226SJed Brown CeedScalar density; 315c677226SJed Brown CeedScalar momentum[3]; 325c677226SJed Brown CeedScalar E_total; 335c677226SJed Brown } StateConservative; 345c677226SJed Brown 355c677226SJed Brown typedef struct { 365c677226SJed Brown StateConservative U; 375c677226SJed Brown StatePrimitive Y; 385c677226SJed Brown } State; 395c677226SJed Brown 405c677226SJed Brown CEED_QFUNCTION_HELPER CeedScalar Dot3(const CeedScalar u[3], 415c677226SJed Brown const CeedScalar v[3]) { 425c677226SJed Brown return u[0]*v[0] + u[1]*v[1] + u[2]*v[2]; 435c677226SJed Brown } 445c677226SJed Brown 455c677226SJed Brown CEED_QFUNCTION_HELPER StatePrimitive StatePrimitiveFromConservative( 465c677226SJed Brown NewtonianIdealGasContext gas, StateConservative U, const CeedScalar x[3]) { 475c677226SJed Brown StatePrimitive Y; 485c677226SJed Brown for (int i=0; i<3; i++) Y.velocity[i] = U.momentum[i] / U.density; 495c677226SJed Brown CeedScalar e_kinetic = .5 * Dot3(Y.velocity, Y.velocity); 505c677226SJed Brown CeedScalar e_potential = -Dot3(gas->g, x); 515c677226SJed Brown CeedScalar e_total = U.E_total / U.density; 525c677226SJed Brown CeedScalar e_internal = e_total - e_kinetic - e_potential; 535c677226SJed Brown Y.temperature = e_internal / gas->cv; 545c677226SJed Brown Y.pressure = (gas->cp / gas->cv - 1) * U.density * e_internal; 555c677226SJed Brown return Y; 565c677226SJed Brown } 575c677226SJed Brown 585c677226SJed Brown CEED_QFUNCTION_HELPER StatePrimitive StatePrimitiveFromConservative_fwd( 595c677226SJed Brown NewtonianIdealGasContext gas, State s, StateConservative dU, 605c677226SJed Brown const CeedScalar x[3], const CeedScalar dx[3]) { 615c677226SJed Brown StatePrimitive dY; 625c677226SJed Brown for (int i=0; i<3; i++) { 635c677226SJed Brown dY.velocity[i] = (dU.momentum[i] - s.Y.velocity[i] * dU.density) / s.U.density; 645c677226SJed Brown } 655c677226SJed Brown CeedScalar e_kinetic = .5 * Dot3(s.Y.velocity, s.Y.velocity); 665c677226SJed Brown CeedScalar de_kinetic = Dot3(dY.velocity, s.Y.velocity); 675c677226SJed Brown CeedScalar e_potential = -Dot3(gas->g, x); 685c677226SJed Brown CeedScalar de_potential = -Dot3(gas->g, dx); 695c677226SJed Brown CeedScalar e_total = s.U.E_total / s.U.density; 705c677226SJed Brown CeedScalar de_total = (dU.E_total - e_total * dU.density) / s.U.density; 715c677226SJed Brown CeedScalar e_internal = e_total - e_kinetic - e_potential; 725c677226SJed Brown CeedScalar de_internal = de_total - de_kinetic - de_potential; 735c677226SJed Brown dY.temperature = de_internal / gas->cv; 745c677226SJed Brown dY.pressure = (gas->cp / gas->cv - 1) 755c677226SJed Brown * (dU.density * e_internal + s.U.density * de_internal); 765c677226SJed Brown return dY; 775c677226SJed Brown } 785c677226SJed Brown 795c677226SJed Brown CEED_QFUNCTION_HELPER State StateFromU(NewtonianIdealGasContext gas, 805c677226SJed Brown const CeedScalar U[5], const CeedScalar x[3]) { 815c677226SJed Brown State s; 825c677226SJed Brown s.U.density = U[0]; 835c677226SJed Brown s.U.momentum[0] = U[1]; 845c677226SJed Brown s.U.momentum[1] = U[2]; 855c677226SJed Brown s.U.momentum[2] = U[3]; 865c677226SJed Brown s.U.E_total = U[4]; 875c677226SJed Brown s.Y = StatePrimitiveFromConservative(gas, s.U, x); 885c677226SJed Brown return s; 895c677226SJed Brown } 905c677226SJed Brown 91*6f00d0e6SJed Brown CEED_QFUNCTION_HELPER State StateFromU_fwd(NewtonianIdealGasContext gas, 92*6f00d0e6SJed Brown State s, const CeedScalar dU[5], 93*6f00d0e6SJed Brown const CeedScalar x[3], const CeedScalar dx[3]) { 94*6f00d0e6SJed Brown State ds; 95*6f00d0e6SJed Brown ds.U.density = dU[0]; 96*6f00d0e6SJed Brown ds.U.momentum[0] = dU[1]; 97*6f00d0e6SJed Brown ds.U.momentum[1] = dU[2]; 98*6f00d0e6SJed Brown ds.U.momentum[2] = dU[3]; 99*6f00d0e6SJed Brown ds.U.E_total = dU[4]; 100*6f00d0e6SJed Brown ds.Y = StatePrimitiveFromConservative_fwd(gas, s, ds.U, x, dx); 101*6f00d0e6SJed Brown return ds; 102*6f00d0e6SJed Brown } 103*6f00d0e6SJed Brown 1045c677226SJed Brown CEED_QFUNCTION_HELPER void FluxInviscid(NewtonianIdealGasContext gas, State s, 1055c677226SJed Brown StateConservative Flux[3]) { 1065c677226SJed Brown for (int i=0; i<3; i++) { 1075c677226SJed Brown Flux[i].density = s.U.momentum[i]; 1085c677226SJed Brown for (int j=0; j<3; j++) 1095c677226SJed Brown Flux[i].momentum[j] = s.U.momentum[i] * s.Y.velocity[j] 1105c677226SJed Brown + s.Y.pressure * (i == j); 1115c677226SJed Brown Flux[i].E_total = (s.U.E_total + s.Y.pressure) * s.Y.velocity[i]; 1125c677226SJed Brown } 1135c677226SJed Brown } 1145c677226SJed Brown 1155c677226SJed Brown CEED_QFUNCTION_HELPER void FluxInviscid_fwd(NewtonianIdealGasContext gas, 1165c677226SJed Brown State s, State ds, StateConservative dFlux[3]) { 1175c677226SJed Brown for (int i=0; i<3; i++) { 1185c677226SJed Brown dFlux[i].density = ds.U.momentum[i]; 1195c677226SJed Brown for (int j=0; j<3; j++) 1205c677226SJed Brown dFlux[i].momentum[j] = ds.U.momentum[i] * s.Y.velocity[j] + 1215c677226SJed Brown s.U.momentum[i] * ds.Y.velocity[j] + ds.Y.pressure * (i == j); 1225c677226SJed Brown dFlux[i].E_total = (ds.U.E_total + ds.Y.pressure) * s.Y.velocity[i] + 1235c677226SJed Brown (s.U.E_total + s.Y.pressure) * ds.Y.velocity[i]; 1245c677226SJed Brown } 1255c677226SJed Brown } 1265c677226SJed Brown 1275c677226SJed Brown // Kelvin-Mandel notation 1285c677226SJed Brown CEED_QFUNCTION_HELPER void KMStrainRate(const State grad_s[3], 1295c677226SJed Brown CeedScalar strain_rate[6]) { 1305c677226SJed Brown const CeedScalar weight = 1 / sqrt(2.); 1315c677226SJed Brown strain_rate[0] = grad_s[0].Y.velocity[0]; 1325c677226SJed Brown strain_rate[1] = grad_s[1].Y.velocity[1]; 1335c677226SJed Brown strain_rate[2] = grad_s[2].Y.velocity[2]; 1345c677226SJed Brown strain_rate[3] = weight * (grad_s[2].Y.velocity[1] + grad_s[1].Y.velocity[2]); 1355c677226SJed Brown strain_rate[4] = weight * (grad_s[2].Y.velocity[0] + grad_s[0].Y.velocity[2]); 1365c677226SJed Brown strain_rate[5] = weight * (grad_s[1].Y.velocity[0] + grad_s[0].Y.velocity[1]); 1375c677226SJed Brown } 1385c677226SJed Brown 1395c677226SJed Brown CEED_QFUNCTION_HELPER void KMUnpack(const CeedScalar v[6], CeedScalar A[3][3]) { 1405c677226SJed Brown const CeedScalar weight = 1 / sqrt(2.); 1415c677226SJed Brown A[0][0] = v[0]; 1425c677226SJed Brown A[1][1] = v[1]; 1435c677226SJed Brown A[2][2] = v[2]; 1445c677226SJed Brown A[2][1] = A[1][2] = weight * v[3]; 1455c677226SJed Brown A[2][0] = A[0][2] = weight * v[4]; 1465c677226SJed Brown A[1][0] = A[0][1] = weight * v[5]; 1475c677226SJed Brown } 1485c677226SJed Brown 1495c677226SJed Brown CEED_QFUNCTION_HELPER void NewtonianStress(NewtonianIdealGasContext gas, 1505c677226SJed Brown const CeedScalar strain_rate[6], CeedScalar stress[6]) { 1515c677226SJed Brown CeedScalar div_u = strain_rate[0] + strain_rate[1] + strain_rate[2]; 1525c677226SJed Brown for (int i=0; i<6; i++) { 1535c677226SJed Brown stress[i] = gas->mu * (2 * strain_rate[i] + gas->lambda * div_u * (i < 3)); 1545c677226SJed Brown } 1555c677226SJed Brown } 1565c677226SJed Brown 1575c677226SJed Brown CEED_QFUNCTION_HELPER void ViscousEnergyFlux(NewtonianIdealGasContext gas, 1585c677226SJed Brown StatePrimitive Y, const State grad_s[3], const CeedScalar stress[3][3], 1595c677226SJed Brown CeedScalar Fe[3]) { 1605c677226SJed Brown for (int i=0; i<3; i++) { 1615c677226SJed Brown Fe[i] = - Y.velocity[0] * stress[0][i] 1625c677226SJed Brown - Y.velocity[1] * stress[1][i] 1635c677226SJed Brown - Y.velocity[2] * stress[2][i] 1645c677226SJed Brown - gas->k * grad_s[i].Y.temperature; 1655c677226SJed Brown } 1665c677226SJed Brown } 1675c677226SJed Brown 16888b783a1SJames Wright // ***************************************************************************** 16988b783a1SJames Wright // Helper function for computing flux Jacobian 17088b783a1SJames Wright // ***************************************************************************** 17188b783a1SJames Wright CEED_QFUNCTION_HELPER void computeFluxJacobian_NS(CeedScalar dF[3][5][5], 17288b783a1SJames Wright const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 17388626eedSJames Wright const CeedScalar gamma, const CeedScalar g[3], const CeedScalar x[3]) { 17488b783a1SJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; // Velocity square 17588626eedSJames Wright CeedScalar e_potential = -(g[0]*x[0] + g[1]*x[1] + g[2]*x[2]); 17688b783a1SJames Wright for (CeedInt i=0; i<3; i++) { // Jacobian matrices for 3 directions 17788b783a1SJames Wright for (CeedInt j=0; j<3; j++) { // Rows of each Jacobian matrix 17888626eedSJames Wright dF[i][j+1][0] = ((i==j) ? ((gamma-1.)*(u_sq/2. - e_potential)) : 0.) - 17988626eedSJames Wright u[i]*u[j]; 18088b783a1SJames Wright for (CeedInt k=0; k<3; k++) { // Columns of each Jacobian matrix 18188b783a1SJames Wright dF[i][0][k+1] = ((i==k) ? 1. : 0.); 18288b783a1SJames Wright dF[i][j+1][k+1] = ((j==k) ? u[i] : 0.) + 18388b783a1SJames Wright ((i==k) ? u[j] : 0.) - 18488b783a1SJames Wright ((i==j) ? u[k] : 0.) * (gamma-1.); 18588b783a1SJames Wright dF[i][4][k+1] = ((i==k) ? (E*gamma/rho - (gamma-1.)*u_sq/2.) : 0.) - 18688b783a1SJames Wright (gamma-1.)*u[i]*u[k]; 18788b783a1SJames Wright } 18888b783a1SJames Wright dF[i][j+1][4] = ((i==j) ? (gamma-1.) : 0.); 18988b783a1SJames Wright } 19088b783a1SJames Wright dF[i][4][0] = u[i] * ((gamma-1.)*u_sq - E*gamma/rho); 19188b783a1SJames Wright dF[i][4][4] = u[i] * gamma; 19288b783a1SJames Wright } 19388b783a1SJames Wright } 19488b783a1SJames Wright 19588b783a1SJames Wright // ***************************************************************************** 19688626eedSJames Wright // Helper function for computing flux Jacobian of Primitive variables 19788626eedSJames Wright // ***************************************************************************** 19888626eedSJames Wright CEED_QFUNCTION_HELPER void computeFluxJacobian_NSp(CeedScalar dF[3][5][5], 19988626eedSJames Wright const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 20088626eedSJames Wright const CeedScalar Rd, const CeedScalar cv) { 20188626eedSJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; // Velocity square 20288626eedSJames Wright // TODO Add in gravity's contribution 20388626eedSJames Wright 20488626eedSJames Wright CeedScalar T = ( E / rho - u_sq / 2. ) / cv; 20588626eedSJames Wright CeedScalar drdT = -rho / T; 20688626eedSJames Wright CeedScalar drdP = 1. / ( Rd * T); 20788626eedSJames Wright CeedScalar etot = E / rho ; 20888626eedSJames Wright CeedScalar e2p = drdP * etot + 1. ; 20988626eedSJames Wright CeedScalar e3p = ( E + rho * Rd * T ); 21088626eedSJames Wright CeedScalar e4p = drdT * etot + rho * cv ; 21188626eedSJames Wright 21288626eedSJames Wright for (CeedInt i=0; i<3; i++) { // Jacobian matrices for 3 directions 21388626eedSJames Wright for (CeedInt j=0; j<3; j++) { // j counts F^{m_j} 21488626eedSJames Wright // [row][col] of A_i 21588626eedSJames Wright dF[i][j+1][0] = drdP * u[i] * u[j] + ((i==j) ? 1. : 0.); // F^{{m_j} wrt p 21688626eedSJames Wright for (CeedInt k=0; k<3; k++) { // k counts the wrt vel_k 217871db79fSKenneth E. Jansen dF[i][0][k+1] = ((i==k) ? rho : 0.); // F^c wrt u_k 21888626eedSJames Wright dF[i][j+1][k+1] = (((j==k) ? u[i] : 0.) + // F^m_j wrt u_k 21988626eedSJames Wright ((i==k) ? u[j] : 0.) ) * rho; 22088626eedSJames Wright dF[i][4][k+1] = rho * u[i] * u[k] 22188626eedSJames Wright + ((i==k) ? e3p : 0.) ; // F^e wrt u_k 22288626eedSJames Wright } 22388626eedSJames Wright dF[i][j+1][4] = drdT * u[i] * u[j]; // F^{m_j} wrt T 22488626eedSJames Wright } 22588626eedSJames Wright dF[i][4][0] = u[i] * e2p; // F^e wrt p 22688626eedSJames Wright dF[i][4][4] = u[i] * e4p; // F^e wrt T 22788626eedSJames Wright dF[i][0][0] = u[i] * drdP; // F^c wrt p 22888626eedSJames Wright dF[i][0][4] = u[i] * drdT; // F^c wrt T 22988626eedSJames Wright } 23088626eedSJames Wright } 23188626eedSJames Wright 23288626eedSJames Wright CEED_QFUNCTION_HELPER void PrimitiveToConservative_fwd(const CeedScalar rho, 23388626eedSJames Wright const CeedScalar u[3], const CeedScalar E, const CeedScalar Rd, 23488626eedSJames Wright const CeedScalar cv, const CeedScalar dY[5], CeedScalar dU[5]) { 23588626eedSJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; 23688626eedSJames Wright CeedScalar T = ( E / rho - u_sq / 2. ) / cv; 23788626eedSJames Wright CeedScalar drdT = -rho / T; 23888626eedSJames Wright CeedScalar drdP = 1. / ( Rd * T); 23988626eedSJames Wright dU[0] = drdP * dY[0] + drdT * dY[4]; 24088626eedSJames Wright CeedScalar de_kinetic = 0; 24188626eedSJames Wright for (int i=0; i<3; i++) { 24288626eedSJames Wright dU[1+i] = dU[0] * u[i] + rho * dY[1+i]; 24388626eedSJames Wright de_kinetic += u[i] * dY[1+i]; 24488626eedSJames Wright } 24588626eedSJames Wright dU[4] = rho * cv * dY[4] + dU[0] * cv * T // internal energy: rho * e 24688626eedSJames Wright + rho * de_kinetic + .5 * dU[0] * u_sq; // kinetic energy: .5 * rho * |u|^2 24788626eedSJames Wright } 24888626eedSJames Wright 24988626eedSJames Wright // ***************************************************************************** 25088626eedSJames Wright // Helper function for computing Tau elements (stabilization constant) 25188626eedSJames Wright // Model from: 25288626eedSJames Wright // PHASTA 25388626eedSJames Wright // 25488626eedSJames Wright // Tau[i] = itau=0 which is diagonal-Shakib (3 values still but not spatial) 25588626eedSJames Wright // 25688626eedSJames Wright // Where NOT UPDATED YET 25788626eedSJames Wright // ***************************************************************************** 25888626eedSJames Wright CEED_QFUNCTION_HELPER void Tau_diagPrim(CeedScalar Tau_d[3], 25988626eedSJames Wright const CeedScalar dXdx[3][3], const CeedScalar u[3], 26088626eedSJames Wright const CeedScalar cv, const NewtonianIdealGasContext newt_ctx, 26188626eedSJames Wright const CeedScalar mu, const CeedScalar dt, 26288626eedSJames Wright const CeedScalar rho) { 26388626eedSJames Wright // Context 26488626eedSJames Wright const CeedScalar Ctau_t = newt_ctx->Ctau_t; 26588626eedSJames Wright const CeedScalar Ctau_v = newt_ctx->Ctau_v; 26688626eedSJames Wright const CeedScalar Ctau_C = newt_ctx->Ctau_C; 26788626eedSJames Wright const CeedScalar Ctau_M = newt_ctx->Ctau_M; 26888626eedSJames Wright const CeedScalar Ctau_E = newt_ctx->Ctau_E; 26988626eedSJames Wright CeedScalar gijd[6]; 27088626eedSJames Wright CeedScalar tau; 27188626eedSJames Wright CeedScalar dts; 27288626eedSJames Wright CeedScalar fact; 27388626eedSJames Wright 27488626eedSJames Wright //*INDENT-OFF* 27588626eedSJames Wright gijd[0] = dXdx[0][0] * dXdx[0][0] 27688626eedSJames Wright + dXdx[1][0] * dXdx[1][0] 27788626eedSJames Wright + dXdx[2][0] * dXdx[2][0]; 27888626eedSJames Wright 27988626eedSJames Wright gijd[1] = dXdx[0][0] * dXdx[0][1] 28088626eedSJames Wright + dXdx[1][0] * dXdx[1][1] 28188626eedSJames Wright + dXdx[2][0] * dXdx[2][1]; 28288626eedSJames Wright 28388626eedSJames Wright gijd[2] = dXdx[0][1] * dXdx[0][1] 28488626eedSJames Wright + dXdx[1][1] * dXdx[1][1] 28588626eedSJames Wright + dXdx[2][1] * dXdx[2][1]; 28688626eedSJames Wright 28788626eedSJames Wright gijd[3] = dXdx[0][0] * dXdx[0][2] 28888626eedSJames Wright + dXdx[1][0] * dXdx[1][2] 28988626eedSJames Wright + dXdx[2][0] * dXdx[2][2]; 29088626eedSJames Wright 29188626eedSJames Wright gijd[4] = dXdx[0][1] * dXdx[0][2] 29288626eedSJames Wright + dXdx[1][1] * dXdx[1][2] 29388626eedSJames Wright + dXdx[2][1] * dXdx[2][2]; 29488626eedSJames Wright 29588626eedSJames Wright gijd[5] = dXdx[0][2] * dXdx[0][2] 29688626eedSJames Wright + dXdx[1][2] * dXdx[1][2] 29788626eedSJames Wright + dXdx[2][2] * dXdx[2][2]; 29888626eedSJames Wright //*INDENT-ON* 29988626eedSJames Wright 30088626eedSJames Wright dts = Ctau_t / dt ; 30188626eedSJames Wright 30288626eedSJames Wright tau = rho*rho*((4. * dts * dts) 30388626eedSJames Wright + u[0] * ( u[0] * gijd[0] + 2. * ( u[1] * gijd[1] + u[2] * gijd[3])) 30488626eedSJames Wright + u[1] * ( u[1] * gijd[2] + 2. * u[2] * gijd[4]) 30588626eedSJames Wright + u[2] * u[2] * gijd[5]) 30688626eedSJames Wright + Ctau_v* mu * mu * 30788626eedSJames Wright (gijd[0]*gijd[0] + gijd[2]*gijd[2] + gijd[5]*gijd[5] + 30888626eedSJames Wright + 2. * (gijd[1]*gijd[1] + gijd[3]*gijd[3] + gijd[4]*gijd[4])); 30988626eedSJames Wright 31088626eedSJames Wright fact=sqrt(tau); 31188626eedSJames Wright 31288626eedSJames Wright Tau_d[0] = Ctau_C * fact / (rho*(gijd[0] + gijd[2] + gijd[5]))*0.125; 31388626eedSJames Wright 31488626eedSJames Wright Tau_d[1] = Ctau_M / fact; 31588626eedSJames Wright Tau_d[2] = Ctau_E / ( fact * cv ); 31688626eedSJames Wright 31788626eedSJames Wright // consider putting back the way I initially had it Ctau_E * Tau_d[1] /cv 31888626eedSJames Wright // to avoid a division if the compiler is smart enough to see that cv IS 31988626eedSJames Wright // a constant that it could invert once for all elements 32088626eedSJames Wright // but in that case energy tau is scaled by the product of Ctau_E * Ctau_M 32188626eedSJames Wright // OR we could absorb cv into Ctau_E but this puts more burden on user to 32288626eedSJames Wright // know how to change constants with a change of fluid or units. Same for 32388626eedSJames Wright // Ctau_v * mu * mu IF AND ONLY IF we don't add viscosity law =f(T) 32488626eedSJames Wright } 32588626eedSJames Wright 32688626eedSJames Wright // ***************************************************************************** 32788b783a1SJames Wright // This QFunction sets a "still" initial condition for generic Newtonian IG problems 32888b783a1SJames Wright // ***************************************************************************** 32988b783a1SJames Wright CEED_QFUNCTION(ICsNewtonianIG)(void *ctx, CeedInt Q, 33088b783a1SJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 33188b783a1SJames Wright // Inputs 33288b783a1SJames Wright const CeedScalar (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 33388b783a1SJames Wright 33488b783a1SJames Wright // Outputs 33588b783a1SJames Wright CeedScalar (*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 33688b783a1SJames Wright 33788626eedSJames Wright // Context 33888626eedSJames Wright const SetupContext context = (SetupContext)ctx; 33988626eedSJames Wright const CeedScalar theta0 = context->theta0; 34088626eedSJames Wright const CeedScalar P0 = context->P0; 34188626eedSJames Wright const CeedScalar cv = context->cv; 34288626eedSJames Wright const CeedScalar cp = context->cp; 34388626eedSJames Wright const CeedScalar *g = context->g; 34488626eedSJames Wright const CeedScalar Rd = cp - cv; 34588626eedSJames Wright 34688b783a1SJames Wright // Quadrature Point Loop 34788b783a1SJames Wright CeedPragmaSIMD 34888b783a1SJames Wright for (CeedInt i=0; i<Q; i++) { 34988b783a1SJames Wright CeedScalar q[5] = {0.}; 35088b783a1SJames Wright 35188b783a1SJames Wright // Setup 35288b783a1SJames Wright // -- Coordinates 35388626eedSJames Wright const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 35488626eedSJames Wright const CeedScalar e_potential = -(g[0]*x[0] + g[1]*x[1] + g[2]*x[2]); 35588b783a1SJames Wright 35688b783a1SJames Wright // -- Density 35788626eedSJames Wright const CeedScalar rho = P0 / (Rd*theta0); 35888b783a1SJames Wright 35988b783a1SJames Wright // Initial Conditions 36088b783a1SJames Wright q[0] = rho; 36188b783a1SJames Wright q[1] = 0.0; 36288b783a1SJames Wright q[2] = 0.0; 36388b783a1SJames Wright q[3] = 0.0; 36488626eedSJames Wright q[4] = rho * (cv*theta0 + e_potential); 36588b783a1SJames Wright 36688b783a1SJames Wright for (CeedInt j=0; j<5; j++) 36788b783a1SJames Wright q0[j][i] = q[j]; 36888b783a1SJames Wright } // End of Quadrature Point Loop 36988b783a1SJames Wright return 0; 37088b783a1SJames Wright } 37188b783a1SJames Wright 37288b783a1SJames Wright // ***************************************************************************** 37388b783a1SJames Wright // This QFunction implements the following formulation of Navier-Stokes with 37488b783a1SJames Wright // explicit time stepping method 37588b783a1SJames Wright // 37688b783a1SJames Wright // This is 3D compressible Navier-Stokes in conservation form with state 37788b783a1SJames Wright // variables of density, momentum density, and total energy density. 37888b783a1SJames Wright // 37988b783a1SJames Wright // State Variables: q = ( rho, U1, U2, U3, E ) 38088b783a1SJames Wright // rho - Mass Density 38188b783a1SJames Wright // Ui - Momentum Density, Ui = rho ui 38288b783a1SJames Wright // E - Total Energy Density, E = rho (cv T + (u u)/2 + g z) 38388b783a1SJames Wright // 38488b783a1SJames Wright // Navier-Stokes Equations: 38588b783a1SJames Wright // drho/dt + div( U ) = 0 38688b783a1SJames Wright // dU/dt + div( rho (u x u) + P I3 ) + rho g khat = div( Fu ) 38788b783a1SJames Wright // dE/dt + div( (E + P) u ) = div( Fe ) 38888b783a1SJames Wright // 38988b783a1SJames Wright // Viscous Stress: 39088b783a1SJames Wright // Fu = mu (grad( u ) + grad( u )^T + lambda div ( u ) I3) 39188b783a1SJames Wright // 39288b783a1SJames Wright // Thermal Stress: 39388b783a1SJames Wright // Fe = u Fu + k grad( T ) 39488626eedSJames Wright // Equation of State 39588b783a1SJames Wright // P = (gamma - 1) (E - rho (u u) / 2 - rho g z) 39688b783a1SJames Wright // 39788b783a1SJames Wright // Stabilization: 39888b783a1SJames Wright // Tau = diag(TauC, TauM, TauM, TauM, TauE) 39988b783a1SJames Wright // f1 = rho sqrt(ui uj gij) 40088b783a1SJames Wright // gij = dXi/dX * dXi/dX 40188b783a1SJames Wright // TauC = Cc f1 / (8 gii) 40288b783a1SJames Wright // TauM = min( 1 , 1 / f1 ) 40388b783a1SJames Wright // TauE = TauM / (Ce cv) 40488b783a1SJames Wright // 40588b783a1SJames Wright // SU = Galerkin + grad(v) . ( Ai^T * Tau * (Aj q,j) ) 40688b783a1SJames Wright // 40788b783a1SJames Wright // Constants: 40888b783a1SJames Wright // lambda = - 2 / 3, From Stokes hypothesis 40988b783a1SJames Wright // mu , Dynamic viscosity 41088b783a1SJames Wright // k , Thermal conductivity 41188b783a1SJames Wright // cv , Specific heat, constant volume 41288b783a1SJames Wright // cp , Specific heat, constant pressure 41388b783a1SJames Wright // g , Gravity 41488b783a1SJames Wright // gamma = cp / cv, Specific heat ratio 41588b783a1SJames Wright // 41688b783a1SJames Wright // We require the product of the inverse of the Jacobian (dXdx_j,k) and 41788b783a1SJames Wright // its transpose (dXdx_k,j) to properly compute integrals of the form: 41888b783a1SJames Wright // int( gradv gradu ) 41988b783a1SJames Wright // 42088b783a1SJames Wright // ***************************************************************************** 4215c677226SJed Brown CEED_QFUNCTION(RHSFunction_Newtonian)(void *ctx, CeedInt Q, 42288b783a1SJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 42388b783a1SJames Wright // *INDENT-OFF* 42488b783a1SJames Wright // Inputs 42588b783a1SJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 42688b783a1SJames Wright (*dq)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 42788b783a1SJames Wright (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 42888b783a1SJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 42988b783a1SJames Wright // Outputs 43088b783a1SJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 43188b783a1SJames Wright (*dv)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1]; 43288b783a1SJames Wright // *INDENT-ON* 43388b783a1SJames Wright 43488b783a1SJames Wright // Context 43588b783a1SJames Wright NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 43688b783a1SJames Wright const CeedScalar mu = context->mu; 43788b783a1SJames Wright const CeedScalar cv = context->cv; 43888b783a1SJames Wright const CeedScalar cp = context->cp; 43988626eedSJames Wright const CeedScalar *g = context->g; 44088626eedSJames Wright const CeedScalar dt = context->dt; 44188b783a1SJames Wright const CeedScalar gamma = cp / cv; 44288626eedSJames Wright const CeedScalar Rd = cp - cv; 44388b783a1SJames Wright 44488b783a1SJames Wright CeedPragmaSIMD 44588b783a1SJames Wright // Quadrature Point Loop 44688b783a1SJames Wright for (CeedInt i=0; i<Q; i++) { 4475c677226SJed Brown CeedScalar U[5]; 4485c677226SJed Brown for (int j=0; j<5; j++) U[j] = q[j][i]; 4495c677226SJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 4505c677226SJed Brown State s = StateFromU(context, U, x_i); 4515c677226SJed Brown 45288b783a1SJames Wright // -- Interp-to-Interp q_data 45388b783a1SJames Wright const CeedScalar wdetJ = q_data[0][i]; 45488b783a1SJames Wright // -- Interp-to-Grad q_data 45588b783a1SJames Wright // ---- Inverse of change of coordinate matrix: X_i,j 45688b783a1SJames Wright // *INDENT-OFF* 45788b783a1SJames Wright const CeedScalar dXdx[3][3] = {{q_data[1][i], 45888b783a1SJames Wright q_data[2][i], 45988b783a1SJames Wright q_data[3][i]}, 46088b783a1SJames Wright {q_data[4][i], 46188b783a1SJames Wright q_data[5][i], 46288b783a1SJames Wright q_data[6][i]}, 46388b783a1SJames Wright {q_data[7][i], 46488b783a1SJames Wright q_data[8][i], 46588b783a1SJames Wright q_data[9][i]} 46688b783a1SJames Wright }; 46788b783a1SJames Wright // *INDENT-ON* 46888b783a1SJames Wright 4695c677226SJed Brown State grad_s[3]; 4705c677226SJed Brown for (int j=0; j<3; j++) { 471*6f00d0e6SJed Brown CeedScalar dx_i[3] = {0}, dU[5]; 472*6f00d0e6SJed Brown for (int k=0; k<5; k++) dU[k] = dq[0][k][i] * dXdx[0][j] 473*6f00d0e6SJed Brown + dq[1][k][i] * dXdx[1][j] 474*6f00d0e6SJed Brown + dq[2][k][i] * dXdx[2][j]; 4755c677226SJed Brown dx_i[j] = 1.; 476*6f00d0e6SJed Brown grad_s[j] = StateFromU_fwd(context, s, dU, x_i, dx_i); 4775c677226SJed Brown } 4785c677226SJed Brown 4795c677226SJed Brown CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 4805c677226SJed Brown KMStrainRate(grad_s, strain_rate); 4815c677226SJed Brown NewtonianStress(context, strain_rate, kmstress); 4825c677226SJed Brown KMUnpack(kmstress, stress); 4835c677226SJed Brown ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 4845c677226SJed Brown 4855c677226SJed Brown StateConservative F_inviscid[3]; 4865c677226SJed Brown FluxInviscid(context, s, F_inviscid); 4875c677226SJed Brown 4885c677226SJed Brown // Total flux 4895c677226SJed Brown CeedScalar Flux[5][3]; 4905c677226SJed Brown for (int j=0; j<3; j++) { 4915c677226SJed Brown Flux[0][j] = F_inviscid[j].density; 4925c677226SJed Brown for (int k=0; k<3; k++) 4935c677226SJed Brown Flux[k+1][j] = F_inviscid[j].momentum[k] - stress[k][j]; 4945c677226SJed Brown Flux[4][j] = F_inviscid[j].E_total + Fe[j]; 4955c677226SJed Brown } 4965c677226SJed Brown 4975c677226SJed Brown for (int j=0; j<3; j++) { 4985c677226SJed Brown for (int k=0; k<5; k++) { 4995c677226SJed Brown dv[j][k][i] = wdetJ * (dXdx[j][0] * Flux[k][0] + 5005c677226SJed Brown dXdx[j][1] * Flux[k][1] + 5015c677226SJed Brown dXdx[j][2] * Flux[k][2]); 5025c677226SJed Brown } 5035c677226SJed Brown } 5045c677226SJed Brown 5055c677226SJed Brown const CeedScalar body_force[5] = {0, s.U.density *g[0], s.U.density *g[1], s.U.density *g[2], 0}; 5065c677226SJed Brown for (int j=0; j<5; j++) 5075c677226SJed Brown v[j][i] = wdetJ * body_force[j]; 50888b783a1SJames Wright 50988b783a1SJames Wright // jacob_F_conv[3][5][5] = dF(convective)/dq at each direction 5105c677226SJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 5115c677226SJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 5125c677226SJed Brown gamma, g, x_i); 5135c677226SJed Brown CeedScalar grad_U[5][3]; 51488b783a1SJames Wright for (int j=0; j<3; j++) { 5155c677226SJed Brown grad_U[0][j] = grad_s[j].U.density; 5165c677226SJed Brown for (int k=0; k<3; k++) grad_U[k+1][j] = grad_s[j].U.momentum[k]; 5175c677226SJed Brown grad_U[4][j] = grad_s[j].U.E_total; 51888b783a1SJames Wright } 51988b783a1SJames Wright 52088b783a1SJames Wright // strong_conv = dF/dq * dq/dx (Strong convection) 52188b783a1SJames Wright CeedScalar strong_conv[5] = {0}; 52288b783a1SJames Wright for (int j=0; j<3; j++) 52388b783a1SJames Wright for (int k=0; k<5; k++) 52488b783a1SJames Wright for (int l=0; l<5; l++) 5255c677226SJed Brown strong_conv[k] += jacob_F_conv[j][k][l] * grad_U[l][j]; 52688b783a1SJames Wright 52788626eedSJames Wright // -- Stabilization method: none, SU, or SUPG 52888626eedSJames Wright CeedScalar stab[5][3] = {{0.}}; 52988626eedSJames Wright CeedScalar tau_strong_conv[5] = {0.}, tau_strong_conv_conservative[5] = {0}; 53088626eedSJames Wright CeedScalar Tau_d[3] = {0.}; 53188b783a1SJames Wright switch (context->stabilization) { 53288b783a1SJames Wright case STAB_NONE: // Galerkin 53388b783a1SJames Wright break; 53488b783a1SJames Wright case STAB_SU: // SU 5355c677226SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 53688626eedSJames Wright tau_strong_conv[0] = Tau_d[0] * strong_conv[0]; 53788626eedSJames Wright tau_strong_conv[1] = Tau_d[1] * strong_conv[1]; 53888626eedSJames Wright tau_strong_conv[2] = Tau_d[1] * strong_conv[2]; 53988626eedSJames Wright tau_strong_conv[3] = Tau_d[1] * strong_conv[3]; 54088626eedSJames Wright tau_strong_conv[4] = Tau_d[2] * strong_conv[4]; 5415c677226SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 5425c677226SJed Brown tau_strong_conv, 54388626eedSJames Wright tau_strong_conv_conservative); 54488b783a1SJames Wright for (int j=0; j<3; j++) 54588b783a1SJames Wright for (int k=0; k<5; k++) 54688b783a1SJames Wright for (int l=0; l<5; l++) 54788626eedSJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_conv_conservative[l]; 54888b783a1SJames Wright 54988b783a1SJames Wright for (int j=0; j<5; j++) 55088b783a1SJames Wright for (int k=0; k<3; k++) 55188b783a1SJames Wright dv[k][j][i] -= wdetJ*(stab[j][0] * dXdx[k][0] + 55288b783a1SJames Wright stab[j][1] * dXdx[k][1] + 55388b783a1SJames Wright stab[j][2] * dXdx[k][2]); 55488b783a1SJames Wright break; 55588b783a1SJames Wright case STAB_SUPG: // SUPG is not implemented for explicit scheme 55688b783a1SJames Wright break; 55788b783a1SJames Wright } 55888b783a1SJames Wright 55988b783a1SJames Wright } // End Quadrature Point Loop 56088b783a1SJames Wright 56188b783a1SJames Wright // Return 56288b783a1SJames Wright return 0; 56388b783a1SJames Wright } 56488b783a1SJames Wright 56588b783a1SJames Wright // ***************************************************************************** 56688b783a1SJames Wright // This QFunction implements the Navier-Stokes equations (mentioned above) with 56788b783a1SJames Wright // implicit time stepping method 56888b783a1SJames Wright // 56988b783a1SJames Wright // SU = Galerkin + grad(v) . ( Ai^T * Tau * (Aj q,j) ) 57088b783a1SJames Wright // SUPG = Galerkin + grad(v) . ( Ai^T * Tau * (q_dot + Aj q,j - body force) ) 57188b783a1SJames Wright // (diffussive terms will be added later) 57288b783a1SJames Wright // 57388b783a1SJames Wright // ***************************************************************************** 57488b783a1SJames Wright CEED_QFUNCTION(IFunction_Newtonian)(void *ctx, CeedInt Q, 57588b783a1SJames Wright const CeedScalar *const *in, 57688b783a1SJames Wright CeedScalar *const *out) { 57788b783a1SJames Wright // *INDENT-OFF* 57888b783a1SJames Wright // Inputs 57988b783a1SJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 58088b783a1SJames Wright (*dq)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 58188b783a1SJames Wright (*q_dot)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 58288b783a1SJames Wright (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3], 58388b783a1SJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[4]; 58488b783a1SJames Wright // Outputs 58588b783a1SJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 58688b783a1SJames Wright (*dv)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1]; 58788b783a1SJames Wright // *INDENT-ON* 58888b783a1SJames Wright // Context 58988b783a1SJames Wright NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 59088b783a1SJames Wright const CeedScalar mu = context->mu; 59188b783a1SJames Wright const CeedScalar cv = context->cv; 59288b783a1SJames Wright const CeedScalar cp = context->cp; 59388626eedSJames Wright const CeedScalar *g = context->g; 59488626eedSJames Wright const CeedScalar dt = context->dt; 59588b783a1SJames Wright const CeedScalar gamma = cp / cv; 59688626eedSJames Wright const CeedScalar Rd = cp-cv; 59788b783a1SJames Wright 59888b783a1SJames Wright CeedPragmaSIMD 59988b783a1SJames Wright // Quadrature Point Loop 60088b783a1SJames Wright for (CeedInt i=0; i<Q; i++) { 6015c677226SJed Brown CeedScalar U[5]; 6025c677226SJed Brown for (int j=0; j<5; j++) U[j] = q[j][i]; 6035c677226SJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 6045c677226SJed Brown State s = StateFromU(context, U, x_i); 6055c677226SJed Brown 60688b783a1SJames Wright // -- Interp-to-Interp q_data 60788b783a1SJames Wright const CeedScalar wdetJ = q_data[0][i]; 60888b783a1SJames Wright // -- Interp-to-Grad q_data 60988b783a1SJames Wright // ---- Inverse of change of coordinate matrix: X_i,j 61088b783a1SJames Wright // *INDENT-OFF* 61188b783a1SJames Wright const CeedScalar dXdx[3][3] = {{q_data[1][i], 61288b783a1SJames Wright q_data[2][i], 61388b783a1SJames Wright q_data[3][i]}, 61488b783a1SJames Wright {q_data[4][i], 61588b783a1SJames Wright q_data[5][i], 61688b783a1SJames Wright q_data[6][i]}, 61788b783a1SJames Wright {q_data[7][i], 61888b783a1SJames Wright q_data[8][i], 61988b783a1SJames Wright q_data[9][i]} 62088b783a1SJames Wright }; 62188b783a1SJames Wright // *INDENT-ON* 6225c677226SJed Brown State grad_s[3]; 62388b783a1SJames Wright for (int j=0; j<3; j++) { 624*6f00d0e6SJed Brown CeedScalar dx_i[3] = {0}, dU[5]; 625*6f00d0e6SJed Brown for (int k=0; k<5; k++) dU[k] = dq[0][k][i] * dXdx[0][j] 626*6f00d0e6SJed Brown + dq[1][k][i] * dXdx[1][j] 627*6f00d0e6SJed Brown + dq[2][k][i] * dXdx[2][j]; 6285c677226SJed Brown dx_i[j] = 1.; 629*6f00d0e6SJed Brown grad_s[j] = StateFromU_fwd(context, s, dU, x_i, dx_i); 63088b783a1SJames Wright } 6315c677226SJed Brown 6325c677226SJed Brown CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 6335c677226SJed Brown KMStrainRate(grad_s, strain_rate); 6345c677226SJed Brown NewtonianStress(context, strain_rate, kmstress); 6355c677226SJed Brown KMUnpack(kmstress, stress); 6365c677226SJed Brown ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 6375c677226SJed Brown 6385c677226SJed Brown StateConservative F_inviscid[3]; 6395c677226SJed Brown FluxInviscid(context, s, F_inviscid); 6405c677226SJed Brown 6415c677226SJed Brown 6425c677226SJed Brown // Total flux 6435c677226SJed Brown CeedScalar Flux[5][3]; 6445c677226SJed Brown for (int j=0; j<3; j++) { 6455c677226SJed Brown Flux[0][j] = F_inviscid[j].density; 64688b783a1SJames Wright for (int k=0; k<3; k++) 6475c677226SJed Brown Flux[k+1][j] = F_inviscid[j].momentum[k] - stress[k][j]; 6485c677226SJed Brown Flux[4][j] = F_inviscid[j].E_total + Fe[j]; 6495c677226SJed Brown } 6505c677226SJed Brown 6515c677226SJed Brown for (int j=0; j<3; j++) { 6525c677226SJed Brown for (int k=0; k<5; k++) { 6535c677226SJed Brown dv[j][k][i] = -wdetJ * (dXdx[j][0] * Flux[k][0] + 6545c677226SJed Brown dXdx[j][1] * Flux[k][1] + 6555c677226SJed Brown dXdx[j][2] * Flux[k][2]); 6565c677226SJed Brown } 6575c677226SJed Brown } 6585c677226SJed Brown 6595c677226SJed Brown const CeedScalar body_force[5] = {0, s.U.density *g[0], s.U.density *g[1], s.U.density *g[2], 0}; 6605c677226SJed Brown for (int j=0; j<5; j++) 6615c677226SJed Brown v[j][i] = wdetJ * (q_dot[j][i] - body_force[j]); 66288b783a1SJames Wright 66388b783a1SJames Wright // jacob_F_conv[3][5][5] = dF(convective)/dq at each direction 6645c677226SJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 6655c677226SJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 6665c677226SJed Brown gamma, g, x_i); 6675c677226SJed Brown CeedScalar grad_U[5][3]; 66888b783a1SJames Wright for (int j=0; j<3; j++) { 6695c677226SJed Brown grad_U[0][j] = grad_s[j].U.density; 6705c677226SJed Brown for (int k=0; k<3; k++) grad_U[k+1][j] = grad_s[j].U.momentum[k]; 6715c677226SJed Brown grad_U[4][j] = grad_s[j].U.E_total; 67288b783a1SJames Wright } 6735c677226SJed Brown 67488b783a1SJames Wright // strong_conv = dF/dq * dq/dx (Strong convection) 67588b783a1SJames Wright CeedScalar strong_conv[5] = {0}; 67688b783a1SJames Wright for (int j=0; j<3; j++) 67788b783a1SJames Wright for (int k=0; k<5; k++) 67888b783a1SJames Wright for (int l=0; l<5; l++) 6795c677226SJed Brown strong_conv[k] += jacob_F_conv[j][k][l] * grad_U[l][j]; 68088b783a1SJames Wright 68188b783a1SJames Wright // Strong residual 68288b783a1SJames Wright CeedScalar strong_res[5]; 68388b783a1SJames Wright for (int j=0; j<5; j++) 68488b783a1SJames Wright strong_res[j] = q_dot[j][i] + strong_conv[j] - body_force[j]; 68588b783a1SJames Wright 68688b783a1SJames Wright // -- Stabilization method: none, SU, or SUPG 68788626eedSJames Wright CeedScalar stab[5][3] = {{0.}}; 68888626eedSJames Wright CeedScalar tau_strong_res[5] = {0.}, tau_strong_res_conservative[5] = {0}; 68988626eedSJames Wright CeedScalar tau_strong_conv[5] = {0.}, tau_strong_conv_conservative[5] = {0}; 69088626eedSJames Wright CeedScalar Tau_d[3] = {0.}; 69188b783a1SJames Wright switch (context->stabilization) { 69288b783a1SJames Wright case STAB_NONE: // Galerkin 69388b783a1SJames Wright break; 69488b783a1SJames Wright case STAB_SU: // SU 6955c677226SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 69688626eedSJames Wright tau_strong_conv[0] = Tau_d[0] * strong_conv[0]; 69788626eedSJames Wright tau_strong_conv[1] = Tau_d[1] * strong_conv[1]; 69888626eedSJames Wright tau_strong_conv[2] = Tau_d[1] * strong_conv[2]; 69988626eedSJames Wright tau_strong_conv[3] = Tau_d[1] * strong_conv[3]; 70088626eedSJames Wright tau_strong_conv[4] = Tau_d[2] * strong_conv[4]; 7015c677226SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 7025c677226SJed Brown tau_strong_conv, tau_strong_conv_conservative); 70388b783a1SJames Wright for (int j=0; j<3; j++) 70488b783a1SJames Wright for (int k=0; k<5; k++) 70588b783a1SJames Wright for (int l=0; l<5; l++) 70688626eedSJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_conv_conservative[l]; 70788b783a1SJames Wright 70888b783a1SJames Wright for (int j=0; j<5; j++) 70988b783a1SJames Wright for (int k=0; k<3; k++) 71088b783a1SJames Wright dv[k][j][i] += wdetJ*(stab[j][0] * dXdx[k][0] + 71188b783a1SJames Wright stab[j][1] * dXdx[k][1] + 71288b783a1SJames Wright stab[j][2] * dXdx[k][2]); 71388b783a1SJames Wright break; 71488b783a1SJames Wright case STAB_SUPG: // SUPG 7155c677226SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 71688626eedSJames Wright tau_strong_res[0] = Tau_d[0] * strong_res[0]; 71788626eedSJames Wright tau_strong_res[1] = Tau_d[1] * strong_res[1]; 71888626eedSJames Wright tau_strong_res[2] = Tau_d[1] * strong_res[2]; 71988626eedSJames Wright tau_strong_res[3] = Tau_d[1] * strong_res[3]; 72088626eedSJames Wright tau_strong_res[4] = Tau_d[2] * strong_res[4]; 72188626eedSJames Wright // Alternate route (useful later with primitive variable code) 72288626eedSJames Wright // this function was verified against PHASTA for as IC that was as close as possible 72388626eedSJames Wright // computeFluxJacobian_NSp(jacob_F_conv_p, rho, u, E, Rd, cv); 72488626eedSJames Wright // it has also been verified to compute a correct through the following 72588626eedSJames Wright // stab[k][j] += jacob_F_conv_p[j][k][l] * tau_strong_res[l] // flux Jacobian wrt primitive 72688626eedSJames Wright // applied in the triple loop below 72788626eedSJames Wright // However, it is more flops than using the existing Jacobian wrt q after q_{,Y} viz 7285c677226SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 7295c677226SJed Brown tau_strong_res, tau_strong_res_conservative); 73088b783a1SJames Wright for (int j=0; j<3; j++) 73188b783a1SJames Wright for (int k=0; k<5; k++) 73288b783a1SJames Wright for (int l=0; l<5; l++) 73388626eedSJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_res_conservative[l]; 73488b783a1SJames Wright 73588b783a1SJames Wright for (int j=0; j<5; j++) 73688b783a1SJames Wright for (int k=0; k<3; k++) 73788b783a1SJames Wright dv[k][j][i] += wdetJ*(stab[j][0] * dXdx[k][0] + 73888b783a1SJames Wright stab[j][1] * dXdx[k][1] + 73988b783a1SJames Wright stab[j][2] * dXdx[k][2]); 74088b783a1SJames Wright break; 74188b783a1SJames Wright } 74288b783a1SJames Wright 74388b783a1SJames Wright } // End Quadrature Point Loop 74488b783a1SJames Wright 74588b783a1SJames Wright // Return 74688b783a1SJames Wright return 0; 74788b783a1SJames Wright } 74888b783a1SJames Wright // ***************************************************************************** 74988b783a1SJames Wright #endif // newtonian_h 750