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" 18c6e8c570SJames Wright #include "newtonian_state.h" 1988b783a1SJames Wright 2088b783a1SJames Wright #ifndef M_PI 2188b783a1SJames Wright #define M_PI 3.14159265358979323846 2288b783a1SJames Wright #endif 2388b783a1SJames Wright 2488b783a1SJames Wright // ***************************************************************************** 2588b783a1SJames Wright // Helper function for computing flux Jacobian 2688b783a1SJames Wright // ***************************************************************************** 2788b783a1SJames Wright CEED_QFUNCTION_HELPER void computeFluxJacobian_NS(CeedScalar dF[3][5][5], 2888b783a1SJames Wright const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 2988626eedSJames Wright const CeedScalar gamma, const CeedScalar g[3], const CeedScalar x[3]) { 3088b783a1SJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; // Velocity square 3188626eedSJames Wright CeedScalar e_potential = -(g[0]*x[0] + g[1]*x[1] + g[2]*x[2]); 3288b783a1SJames Wright for (CeedInt i=0; i<3; i++) { // Jacobian matrices for 3 directions 3388b783a1SJames Wright for (CeedInt j=0; j<3; j++) { // Rows of each Jacobian matrix 3488626eedSJames Wright dF[i][j+1][0] = ((i==j) ? ((gamma-1.)*(u_sq/2. - e_potential)) : 0.) - 3588626eedSJames Wright u[i]*u[j]; 3688b783a1SJames Wright for (CeedInt k=0; k<3; k++) { // Columns of each Jacobian matrix 3788b783a1SJames Wright dF[i][0][k+1] = ((i==k) ? 1. : 0.); 3888b783a1SJames Wright dF[i][j+1][k+1] = ((j==k) ? u[i] : 0.) + 3988b783a1SJames Wright ((i==k) ? u[j] : 0.) - 4088b783a1SJames Wright ((i==j) ? u[k] : 0.) * (gamma-1.); 4188b783a1SJames Wright dF[i][4][k+1] = ((i==k) ? (E*gamma/rho - (gamma-1.)*u_sq/2.) : 0.) - 4288b783a1SJames Wright (gamma-1.)*u[i]*u[k]; 4388b783a1SJames Wright } 4488b783a1SJames Wright dF[i][j+1][4] = ((i==j) ? (gamma-1.) : 0.); 4588b783a1SJames Wright } 4688b783a1SJames Wright dF[i][4][0] = u[i] * ((gamma-1.)*u_sq - E*gamma/rho); 4788b783a1SJames Wright dF[i][4][4] = u[i] * gamma; 4888b783a1SJames Wright } 4988b783a1SJames Wright } 5088b783a1SJames Wright 5188b783a1SJames Wright // ***************************************************************************** 5288626eedSJames Wright // Helper function for computing flux Jacobian of Primitive variables 5388626eedSJames Wright // ***************************************************************************** 5488626eedSJames Wright CEED_QFUNCTION_HELPER void computeFluxJacobian_NSp(CeedScalar dF[3][5][5], 5588626eedSJames Wright const CeedScalar rho, const CeedScalar u[3], const CeedScalar E, 5688626eedSJames Wright const CeedScalar Rd, const CeedScalar cv) { 5788626eedSJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; // Velocity square 5888626eedSJames Wright // TODO Add in gravity's contribution 5988626eedSJames Wright 6088626eedSJames Wright CeedScalar T = ( E / rho - u_sq / 2. ) / cv; 6188626eedSJames Wright CeedScalar drdT = -rho / T; 6288626eedSJames Wright CeedScalar drdP = 1. / ( Rd * T); 6388626eedSJames Wright CeedScalar etot = E / rho ; 6488626eedSJames Wright CeedScalar e2p = drdP * etot + 1. ; 6588626eedSJames Wright CeedScalar e3p = ( E + rho * Rd * T ); 6688626eedSJames Wright CeedScalar e4p = drdT * etot + rho * cv ; 6788626eedSJames Wright 6888626eedSJames Wright for (CeedInt i=0; i<3; i++) { // Jacobian matrices for 3 directions 6988626eedSJames Wright for (CeedInt j=0; j<3; j++) { // j counts F^{m_j} 7088626eedSJames Wright // [row][col] of A_i 7188626eedSJames Wright dF[i][j+1][0] = drdP * u[i] * u[j] + ((i==j) ? 1. : 0.); // F^{{m_j} wrt p 7288626eedSJames Wright for (CeedInt k=0; k<3; k++) { // k counts the wrt vel_k 73871db79fSKenneth E. Jansen dF[i][0][k+1] = ((i==k) ? rho : 0.); // F^c wrt u_k 7488626eedSJames Wright dF[i][j+1][k+1] = (((j==k) ? u[i] : 0.) + // F^m_j wrt u_k 7588626eedSJames Wright ((i==k) ? u[j] : 0.) ) * rho; 7688626eedSJames Wright dF[i][4][k+1] = rho * u[i] * u[k] 7788626eedSJames Wright + ((i==k) ? e3p : 0.) ; // F^e wrt u_k 7888626eedSJames Wright } 7988626eedSJames Wright dF[i][j+1][4] = drdT * u[i] * u[j]; // F^{m_j} wrt T 8088626eedSJames Wright } 8188626eedSJames Wright dF[i][4][0] = u[i] * e2p; // F^e wrt p 8288626eedSJames Wright dF[i][4][4] = u[i] * e4p; // F^e wrt T 8388626eedSJames Wright dF[i][0][0] = u[i] * drdP; // F^c wrt p 8488626eedSJames Wright dF[i][0][4] = u[i] * drdT; // F^c wrt T 8588626eedSJames Wright } 8688626eedSJames Wright } 8788626eedSJames Wright 8888626eedSJames Wright CEED_QFUNCTION_HELPER void PrimitiveToConservative_fwd(const CeedScalar rho, 8988626eedSJames Wright const CeedScalar u[3], const CeedScalar E, const CeedScalar Rd, 9088626eedSJames Wright const CeedScalar cv, const CeedScalar dY[5], CeedScalar dU[5]) { 9188626eedSJames Wright CeedScalar u_sq = u[0]*u[0] + u[1]*u[1] + u[2]*u[2]; 9288626eedSJames Wright CeedScalar T = ( E / rho - u_sq / 2. ) / cv; 9388626eedSJames Wright CeedScalar drdT = -rho / T; 9488626eedSJames Wright CeedScalar drdP = 1. / ( Rd * T); 9588626eedSJames Wright dU[0] = drdP * dY[0] + drdT * dY[4]; 9688626eedSJames Wright CeedScalar de_kinetic = 0; 97ba6664aeSJames Wright for (CeedInt i=0; i<3; i++) { 9888626eedSJames Wright dU[1+i] = dU[0] * u[i] + rho * dY[1+i]; 9988626eedSJames Wright de_kinetic += u[i] * dY[1+i]; 10088626eedSJames Wright } 10188626eedSJames Wright dU[4] = rho * cv * dY[4] + dU[0] * cv * T // internal energy: rho * e 10288626eedSJames Wright + rho * de_kinetic + .5 * dU[0] * u_sq; // kinetic energy: .5 * rho * |u|^2 10388626eedSJames Wright } 10488626eedSJames Wright 10588626eedSJames Wright // ***************************************************************************** 10688626eedSJames Wright // Helper function for computing Tau elements (stabilization constant) 10788626eedSJames Wright // Model from: 10888626eedSJames Wright // PHASTA 10988626eedSJames Wright // 11088626eedSJames Wright // Tau[i] = itau=0 which is diagonal-Shakib (3 values still but not spatial) 11188626eedSJames Wright // 11288626eedSJames Wright // Where NOT UPDATED YET 11388626eedSJames Wright // ***************************************************************************** 11488626eedSJames Wright CEED_QFUNCTION_HELPER void Tau_diagPrim(CeedScalar Tau_d[3], 11588626eedSJames Wright const CeedScalar dXdx[3][3], const CeedScalar u[3], 11688626eedSJames Wright const CeedScalar cv, const NewtonianIdealGasContext newt_ctx, 11788626eedSJames Wright const CeedScalar mu, const CeedScalar dt, 11888626eedSJames Wright const CeedScalar rho) { 11988626eedSJames Wright // Context 12088626eedSJames Wright const CeedScalar Ctau_t = newt_ctx->Ctau_t; 12188626eedSJames Wright const CeedScalar Ctau_v = newt_ctx->Ctau_v; 12288626eedSJames Wright const CeedScalar Ctau_C = newt_ctx->Ctau_C; 12388626eedSJames Wright const CeedScalar Ctau_M = newt_ctx->Ctau_M; 12488626eedSJames Wright const CeedScalar Ctau_E = newt_ctx->Ctau_E; 12588626eedSJames Wright CeedScalar gijd[6]; 12688626eedSJames Wright CeedScalar tau; 12788626eedSJames Wright CeedScalar dts; 12888626eedSJames Wright CeedScalar fact; 12988626eedSJames Wright 13088626eedSJames Wright //*INDENT-OFF* 13188626eedSJames Wright gijd[0] = dXdx[0][0] * dXdx[0][0] 13288626eedSJames Wright + dXdx[1][0] * dXdx[1][0] 13388626eedSJames Wright + dXdx[2][0] * dXdx[2][0]; 13488626eedSJames Wright 13588626eedSJames Wright gijd[1] = dXdx[0][0] * dXdx[0][1] 13688626eedSJames Wright + dXdx[1][0] * dXdx[1][1] 13788626eedSJames Wright + dXdx[2][0] * dXdx[2][1]; 13888626eedSJames Wright 13988626eedSJames Wright gijd[2] = dXdx[0][1] * dXdx[0][1] 14088626eedSJames Wright + dXdx[1][1] * dXdx[1][1] 14188626eedSJames Wright + dXdx[2][1] * dXdx[2][1]; 14288626eedSJames Wright 14388626eedSJames Wright gijd[3] = dXdx[0][0] * dXdx[0][2] 14488626eedSJames Wright + dXdx[1][0] * dXdx[1][2] 14588626eedSJames Wright + dXdx[2][0] * dXdx[2][2]; 14688626eedSJames Wright 14788626eedSJames Wright gijd[4] = dXdx[0][1] * dXdx[0][2] 14888626eedSJames Wright + dXdx[1][1] * dXdx[1][2] 14988626eedSJames Wright + dXdx[2][1] * dXdx[2][2]; 15088626eedSJames Wright 15188626eedSJames Wright gijd[5] = dXdx[0][2] * dXdx[0][2] 15288626eedSJames Wright + dXdx[1][2] * dXdx[1][2] 15388626eedSJames Wright + dXdx[2][2] * dXdx[2][2]; 15488626eedSJames Wright //*INDENT-ON* 15588626eedSJames Wright 15688626eedSJames Wright dts = Ctau_t / dt ; 15788626eedSJames Wright 15888626eedSJames Wright tau = rho*rho*((4. * dts * dts) 15988626eedSJames Wright + u[0] * ( u[0] * gijd[0] + 2. * ( u[1] * gijd[1] + u[2] * gijd[3])) 16088626eedSJames Wright + u[1] * ( u[1] * gijd[2] + 2. * u[2] * gijd[4]) 16188626eedSJames Wright + u[2] * u[2] * gijd[5]) 16288626eedSJames Wright + Ctau_v* mu * mu * 16388626eedSJames Wright (gijd[0]*gijd[0] + gijd[2]*gijd[2] + gijd[5]*gijd[5] + 16488626eedSJames Wright + 2. * (gijd[1]*gijd[1] + gijd[3]*gijd[3] + gijd[4]*gijd[4])); 16588626eedSJames Wright 16688626eedSJames Wright fact=sqrt(tau); 16788626eedSJames Wright 16888626eedSJames Wright Tau_d[0] = Ctau_C * fact / (rho*(gijd[0] + gijd[2] + gijd[5]))*0.125; 16988626eedSJames Wright 17088626eedSJames Wright Tau_d[1] = Ctau_M / fact; 17188626eedSJames Wright Tau_d[2] = Ctau_E / ( fact * cv ); 17288626eedSJames Wright 17388626eedSJames Wright // consider putting back the way I initially had it Ctau_E * Tau_d[1] /cv 17488626eedSJames Wright // to avoid a division if the compiler is smart enough to see that cv IS 17588626eedSJames Wright // a constant that it could invert once for all elements 17688626eedSJames Wright // but in that case energy tau is scaled by the product of Ctau_E * Ctau_M 17788626eedSJames Wright // OR we could absorb cv into Ctau_E but this puts more burden on user to 17888626eedSJames Wright // know how to change constants with a change of fluid or units. Same for 17988626eedSJames Wright // Ctau_v * mu * mu IF AND ONLY IF we don't add viscosity law =f(T) 18088626eedSJames Wright } 18188626eedSJames Wright 18288626eedSJames Wright // ***************************************************************************** 18388b783a1SJames Wright // This QFunction sets a "still" initial condition for generic Newtonian IG problems 18488b783a1SJames Wright // ***************************************************************************** 18588b783a1SJames Wright CEED_QFUNCTION(ICsNewtonianIG)(void *ctx, CeedInt Q, 18688b783a1SJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 18788b783a1SJames Wright // Inputs 18888b783a1SJames Wright const CeedScalar (*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0]; 18988b783a1SJames Wright 19088b783a1SJames Wright // Outputs 19188b783a1SJames Wright CeedScalar (*q0)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 19288b783a1SJames Wright 19388626eedSJames Wright // Context 19488626eedSJames Wright const SetupContext context = (SetupContext)ctx; 19588626eedSJames Wright const CeedScalar theta0 = context->theta0; 19688626eedSJames Wright const CeedScalar P0 = context->P0; 19788626eedSJames Wright const CeedScalar cv = context->cv; 19888626eedSJames Wright const CeedScalar cp = context->cp; 19988626eedSJames Wright const CeedScalar *g = context->g; 20088626eedSJames Wright const CeedScalar Rd = cp - cv; 20188626eedSJames Wright 20288b783a1SJames Wright // Quadrature Point Loop 20388b783a1SJames Wright CeedPragmaSIMD 20488b783a1SJames Wright for (CeedInt i=0; i<Q; i++) { 20588b783a1SJames Wright CeedScalar q[5] = {0.}; 20688b783a1SJames Wright 20788b783a1SJames Wright // Setup 20888b783a1SJames Wright // -- Coordinates 20988626eedSJames Wright const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]}; 21088626eedSJames Wright const CeedScalar e_potential = -(g[0]*x[0] + g[1]*x[1] + g[2]*x[2]); 21188b783a1SJames Wright 21288b783a1SJames Wright // -- Density 21388626eedSJames Wright const CeedScalar rho = P0 / (Rd*theta0); 21488b783a1SJames Wright 21588b783a1SJames Wright // Initial Conditions 21688b783a1SJames Wright q[0] = rho; 21788b783a1SJames Wright q[1] = 0.0; 21888b783a1SJames Wright q[2] = 0.0; 21988b783a1SJames Wright q[3] = 0.0; 22088626eedSJames Wright q[4] = rho * (cv*theta0 + e_potential); 22188b783a1SJames Wright 22288b783a1SJames Wright for (CeedInt j=0; j<5; j++) 22388b783a1SJames Wright q0[j][i] = q[j]; 22488b783a1SJames Wright } // End of Quadrature Point Loop 22588b783a1SJames Wright return 0; 22688b783a1SJames Wright } 22788b783a1SJames Wright 22888b783a1SJames Wright // ***************************************************************************** 22988b783a1SJames Wright // This QFunction implements the following formulation of Navier-Stokes with 23088b783a1SJames Wright // explicit time stepping method 23188b783a1SJames Wright // 23288b783a1SJames Wright // This is 3D compressible Navier-Stokes in conservation form with state 23388b783a1SJames Wright // variables of density, momentum density, and total energy density. 23488b783a1SJames Wright // 23588b783a1SJames Wright // State Variables: q = ( rho, U1, U2, U3, E ) 23688b783a1SJames Wright // rho - Mass Density 23788b783a1SJames Wright // Ui - Momentum Density, Ui = rho ui 23888b783a1SJames Wright // E - Total Energy Density, E = rho (cv T + (u u)/2 + g z) 23988b783a1SJames Wright // 24088b783a1SJames Wright // Navier-Stokes Equations: 24188b783a1SJames Wright // drho/dt + div( U ) = 0 24288b783a1SJames Wright // dU/dt + div( rho (u x u) + P I3 ) + rho g khat = div( Fu ) 24388b783a1SJames Wright // dE/dt + div( (E + P) u ) = div( Fe ) 24488b783a1SJames Wright // 24588b783a1SJames Wright // Viscous Stress: 24688b783a1SJames Wright // Fu = mu (grad( u ) + grad( u )^T + lambda div ( u ) I3) 24788b783a1SJames Wright // 24888b783a1SJames Wright // Thermal Stress: 24988b783a1SJames Wright // Fe = u Fu + k grad( T ) 25088626eedSJames Wright // Equation of State 25188b783a1SJames Wright // P = (gamma - 1) (E - rho (u u) / 2 - rho g z) 25288b783a1SJames Wright // 25388b783a1SJames Wright // Stabilization: 25488b783a1SJames Wright // Tau = diag(TauC, TauM, TauM, TauM, TauE) 25588b783a1SJames Wright // f1 = rho sqrt(ui uj gij) 25688b783a1SJames Wright // gij = dXi/dX * dXi/dX 25788b783a1SJames Wright // TauC = Cc f1 / (8 gii) 25888b783a1SJames Wright // TauM = min( 1 , 1 / f1 ) 25988b783a1SJames Wright // TauE = TauM / (Ce cv) 26088b783a1SJames Wright // 26188b783a1SJames Wright // SU = Galerkin + grad(v) . ( Ai^T * Tau * (Aj q,j) ) 26288b783a1SJames Wright // 26388b783a1SJames Wright // Constants: 26488b783a1SJames Wright // lambda = - 2 / 3, From Stokes hypothesis 26588b783a1SJames Wright // mu , Dynamic viscosity 26688b783a1SJames Wright // k , Thermal conductivity 26788b783a1SJames Wright // cv , Specific heat, constant volume 26888b783a1SJames Wright // cp , Specific heat, constant pressure 26988b783a1SJames Wright // g , Gravity 27088b783a1SJames Wright // gamma = cp / cv, Specific heat ratio 27188b783a1SJames Wright // 27288b783a1SJames Wright // We require the product of the inverse of the Jacobian (dXdx_j,k) and 27388b783a1SJames Wright // its transpose (dXdx_k,j) to properly compute integrals of the form: 27488b783a1SJames Wright // int( gradv gradu ) 27588b783a1SJames Wright // 27688b783a1SJames Wright // ***************************************************************************** 2775c677226SJed Brown CEED_QFUNCTION(RHSFunction_Newtonian)(void *ctx, CeedInt Q, 27888b783a1SJames Wright const CeedScalar *const *in, CeedScalar *const *out) { 27988b783a1SJames Wright // *INDENT-OFF* 28088b783a1SJames Wright // Inputs 28188b783a1SJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 282a3ae0734SJed Brown (*Grad_q)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 28388b783a1SJames Wright (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 28488b783a1SJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 28588b783a1SJames Wright // Outputs 28688b783a1SJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 287a3ae0734SJed Brown (*Grad_v)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1]; 28888b783a1SJames Wright // *INDENT-ON* 28988b783a1SJames Wright 29088b783a1SJames Wright // Context 29188b783a1SJames Wright NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 29288b783a1SJames Wright const CeedScalar mu = context->mu; 29388b783a1SJames Wright const CeedScalar cv = context->cv; 29488b783a1SJames Wright const CeedScalar cp = context->cp; 29588626eedSJames Wright const CeedScalar *g = context->g; 29688626eedSJames Wright const CeedScalar dt = context->dt; 29788b783a1SJames Wright const CeedScalar gamma = cp / cv; 29888626eedSJames Wright const CeedScalar Rd = cp - cv; 29988b783a1SJames Wright 30088b783a1SJames Wright CeedPragmaSIMD 30188b783a1SJames Wright // Quadrature Point Loop 30288b783a1SJames Wright for (CeedInt i=0; i<Q; i++) { 3035c677226SJed Brown CeedScalar U[5]; 3045c677226SJed Brown for (int j=0; j<5; j++) U[j] = q[j][i]; 3055c677226SJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 3065c677226SJed Brown State s = StateFromU(context, U, x_i); 3075c677226SJed Brown 30888b783a1SJames Wright // -- Interp-to-Interp q_data 30988b783a1SJames Wright const CeedScalar wdetJ = q_data[0][i]; 31088b783a1SJames Wright // -- Interp-to-Grad q_data 31188b783a1SJames Wright // ---- Inverse of change of coordinate matrix: X_i,j 31288b783a1SJames Wright // *INDENT-OFF* 31388b783a1SJames Wright const CeedScalar dXdx[3][3] = {{q_data[1][i], 31488b783a1SJames Wright q_data[2][i], 31588b783a1SJames Wright q_data[3][i]}, 31688b783a1SJames Wright {q_data[4][i], 31788b783a1SJames Wright q_data[5][i], 31888b783a1SJames Wright q_data[6][i]}, 31988b783a1SJames Wright {q_data[7][i], 32088b783a1SJames Wright q_data[8][i], 32188b783a1SJames Wright q_data[9][i]} 32288b783a1SJames Wright }; 32388b783a1SJames Wright // *INDENT-ON* 32488b783a1SJames Wright 3255c677226SJed Brown State grad_s[3]; 3263c4b7af6SJed Brown for (CeedInt j=0; j<3; j++) { 3276f00d0e6SJed Brown CeedScalar dx_i[3] = {0}, dU[5]; 32839c69132SJed Brown for (CeedInt k=0; k<5; k++) 32939c69132SJed Brown dU[k] = Grad_q[0][k][i] * dXdx[0][j] + 33039c69132SJed Brown Grad_q[1][k][i] * dXdx[1][j] + 33139c69132SJed Brown Grad_q[2][k][i] * dXdx[2][j]; 3325c677226SJed Brown dx_i[j] = 1.; 3336f00d0e6SJed Brown grad_s[j] = StateFromU_fwd(context, s, dU, x_i, dx_i); 3345c677226SJed Brown } 3355c677226SJed Brown 3365c677226SJed Brown CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 3375c677226SJed Brown KMStrainRate(grad_s, strain_rate); 3385c677226SJed Brown NewtonianStress(context, strain_rate, kmstress); 3395c677226SJed Brown KMUnpack(kmstress, stress); 3405c677226SJed Brown ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 3415c677226SJed Brown 3425c677226SJed Brown StateConservative F_inviscid[3]; 3435c677226SJed Brown FluxInviscid(context, s, F_inviscid); 3445c677226SJed Brown 3455c677226SJed Brown // Total flux 3465c677226SJed Brown CeedScalar Flux[5][3]; 3473c4b7af6SJed Brown for (CeedInt j=0; j<3; j++) { 3485c677226SJed Brown Flux[0][j] = F_inviscid[j].density; 3493c4b7af6SJed Brown for (CeedInt k=0; k<3; k++) 3505c677226SJed Brown Flux[k+1][j] = F_inviscid[j].momentum[k] - stress[k][j]; 3515c677226SJed Brown Flux[4][j] = F_inviscid[j].E_total + Fe[j]; 3525c677226SJed Brown } 3535c677226SJed Brown 3543c4b7af6SJed Brown for (CeedInt j=0; j<3; j++) { 3553c4b7af6SJed Brown for (CeedInt k=0; k<5; k++) { 356a3ae0734SJed Brown Grad_v[j][k][i] = wdetJ * (dXdx[j][0] * Flux[k][0] + 3575c677226SJed Brown dXdx[j][1] * Flux[k][1] + 3585c677226SJed Brown dXdx[j][2] * Flux[k][2]); 3595c677226SJed Brown } 3605c677226SJed Brown } 3615c677226SJed Brown 3625c677226SJed Brown const CeedScalar body_force[5] = {0, s.U.density *g[0], s.U.density *g[1], s.U.density *g[2], 0}; 3635c677226SJed Brown for (int j=0; j<5; j++) 3645c677226SJed Brown v[j][i] = wdetJ * body_force[j]; 36588b783a1SJames Wright 36688b783a1SJames Wright // jacob_F_conv[3][5][5] = dF(convective)/dq at each direction 3675c677226SJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 3685c677226SJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 3695c677226SJed Brown gamma, g, x_i); 3705c677226SJed Brown CeedScalar grad_U[5][3]; 371ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) { 3725c677226SJed Brown grad_U[0][j] = grad_s[j].U.density; 3733c4b7af6SJed Brown for (CeedInt k=0; k<3; k++) grad_U[k+1][j] = grad_s[j].U.momentum[k]; 3745c677226SJed Brown grad_U[4][j] = grad_s[j].U.E_total; 37588b783a1SJames Wright } 37688b783a1SJames Wright 37788b783a1SJames Wright // strong_conv = dF/dq * dq/dx (Strong convection) 37888b783a1SJames Wright CeedScalar strong_conv[5] = {0}; 379ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) 380ba6664aeSJames Wright for (CeedInt k=0; k<5; k++) 381ba6664aeSJames Wright for (CeedInt l=0; l<5; l++) 3825c677226SJed Brown strong_conv[k] += jacob_F_conv[j][k][l] * grad_U[l][j]; 38388b783a1SJames Wright 38488626eedSJames Wright // -- Stabilization method: none, SU, or SUPG 38588626eedSJames Wright CeedScalar stab[5][3] = {{0.}}; 38688626eedSJames Wright CeedScalar tau_strong_conv[5] = {0.}, tau_strong_conv_conservative[5] = {0}; 38788626eedSJames Wright CeedScalar Tau_d[3] = {0.}; 38888b783a1SJames Wright switch (context->stabilization) { 38988b783a1SJames Wright case STAB_NONE: // Galerkin 39088b783a1SJames Wright break; 39188b783a1SJames Wright case STAB_SU: // SU 3925c677226SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 39388626eedSJames Wright tau_strong_conv[0] = Tau_d[0] * strong_conv[0]; 39488626eedSJames Wright tau_strong_conv[1] = Tau_d[1] * strong_conv[1]; 39588626eedSJames Wright tau_strong_conv[2] = Tau_d[1] * strong_conv[2]; 39688626eedSJames Wright tau_strong_conv[3] = Tau_d[1] * strong_conv[3]; 39788626eedSJames Wright tau_strong_conv[4] = Tau_d[2] * strong_conv[4]; 3985c677226SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 3995c677226SJed Brown tau_strong_conv, 40088626eedSJames Wright tau_strong_conv_conservative); 401ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) 402ba6664aeSJames Wright for (CeedInt k=0; k<5; k++) 403ba6664aeSJames Wright for (CeedInt l=0; l<5; l++) 40488626eedSJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_conv_conservative[l]; 40588b783a1SJames Wright 406ba6664aeSJames Wright for (CeedInt j=0; j<5; j++) 407ba6664aeSJames Wright for (CeedInt k=0; k<3; k++) 408a3ae0734SJed Brown Grad_v[k][j][i] -= wdetJ*(stab[j][0] * dXdx[k][0] + 40988b783a1SJames Wright stab[j][1] * dXdx[k][1] + 41088b783a1SJames Wright stab[j][2] * dXdx[k][2]); 41188b783a1SJames Wright break; 41288b783a1SJames Wright case STAB_SUPG: // SUPG is not implemented for explicit scheme 41388b783a1SJames Wright break; 41488b783a1SJames Wright } 41588b783a1SJames Wright 41688b783a1SJames Wright } // End Quadrature Point Loop 41788b783a1SJames Wright 41888b783a1SJames Wright // Return 41988b783a1SJames Wright return 0; 42088b783a1SJames Wright } 42188b783a1SJames Wright 42288b783a1SJames Wright // ***************************************************************************** 42388b783a1SJames Wright // This QFunction implements the Navier-Stokes equations (mentioned above) with 42488b783a1SJames Wright // implicit time stepping method 42588b783a1SJames Wright // 42688b783a1SJames Wright // SU = Galerkin + grad(v) . ( Ai^T * Tau * (Aj q,j) ) 42788b783a1SJames Wright // SUPG = Galerkin + grad(v) . ( Ai^T * Tau * (q_dot + Aj q,j - body force) ) 42888b783a1SJames Wright // (diffussive terms will be added later) 42988b783a1SJames Wright // 43088b783a1SJames Wright // ***************************************************************************** 43188b783a1SJames Wright CEED_QFUNCTION(IFunction_Newtonian)(void *ctx, CeedInt Q, 43288b783a1SJames Wright const CeedScalar *const *in, 43388b783a1SJames Wright CeedScalar *const *out) { 43488b783a1SJames Wright // *INDENT-OFF* 43588b783a1SJames Wright // Inputs 43688b783a1SJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 437a3ae0734SJed Brown (*Grad_q)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 43888b783a1SJames Wright (*q_dot)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 43988b783a1SJames Wright (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3], 44088b783a1SJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[4]; 44188b783a1SJames Wright // Outputs 44288b783a1SJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 443a3ae0734SJed Brown (*Grad_v)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1], 444a3ae0734SJed Brown (*jac_data)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[2]; 44588b783a1SJames Wright // *INDENT-ON* 44688b783a1SJames Wright // Context 44788b783a1SJames Wright NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 44888b783a1SJames Wright const CeedScalar mu = context->mu; 44988b783a1SJames Wright const CeedScalar cv = context->cv; 45088b783a1SJames Wright const CeedScalar cp = context->cp; 45188626eedSJames Wright const CeedScalar *g = context->g; 45288626eedSJames Wright const CeedScalar dt = context->dt; 45388b783a1SJames Wright const CeedScalar gamma = cp / cv; 45488626eedSJames Wright const CeedScalar Rd = cp-cv; 45588b783a1SJames Wright 45688b783a1SJames Wright CeedPragmaSIMD 45788b783a1SJames Wright // Quadrature Point Loop 45888b783a1SJames Wright for (CeedInt i=0; i<Q; i++) { 4595c677226SJed Brown CeedScalar U[5]; 4603c4b7af6SJed Brown for (CeedInt j=0; j<5; j++) U[j] = q[j][i]; 4615c677226SJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 4625c677226SJed Brown State s = StateFromU(context, U, x_i); 4635c677226SJed Brown 46488b783a1SJames Wright // -- Interp-to-Interp q_data 46588b783a1SJames Wright const CeedScalar wdetJ = q_data[0][i]; 46688b783a1SJames Wright // -- Interp-to-Grad q_data 46788b783a1SJames Wright // ---- Inverse of change of coordinate matrix: X_i,j 46888b783a1SJames Wright // *INDENT-OFF* 46988b783a1SJames Wright const CeedScalar dXdx[3][3] = {{q_data[1][i], 47088b783a1SJames Wright q_data[2][i], 47188b783a1SJames Wright q_data[3][i]}, 47288b783a1SJames Wright {q_data[4][i], 47388b783a1SJames Wright q_data[5][i], 47488b783a1SJames Wright q_data[6][i]}, 47588b783a1SJames Wright {q_data[7][i], 47688b783a1SJames Wright q_data[8][i], 47788b783a1SJames Wright q_data[9][i]} 47888b783a1SJames Wright }; 47988b783a1SJames Wright // *INDENT-ON* 4805c677226SJed Brown State grad_s[3]; 481ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) { 4826f00d0e6SJed Brown CeedScalar dx_i[3] = {0}, dU[5]; 48339c69132SJed Brown for (CeedInt k=0; k<5; k++) 48439c69132SJed Brown dU[k] = Grad_q[0][k][i] * dXdx[0][j] + 48539c69132SJed Brown Grad_q[1][k][i] * dXdx[1][j] + 48639c69132SJed Brown Grad_q[2][k][i] * dXdx[2][j]; 4875c677226SJed Brown dx_i[j] = 1.; 4886f00d0e6SJed Brown grad_s[j] = StateFromU_fwd(context, s, dU, x_i, dx_i); 48988b783a1SJames Wright } 4905c677226SJed Brown 4915c677226SJed Brown CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 4925c677226SJed Brown KMStrainRate(grad_s, strain_rate); 4935c677226SJed Brown NewtonianStress(context, strain_rate, kmstress); 4945c677226SJed Brown KMUnpack(kmstress, stress); 4955c677226SJed Brown ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 4965c677226SJed Brown 4975c677226SJed Brown StateConservative F_inviscid[3]; 4985c677226SJed Brown FluxInviscid(context, s, F_inviscid); 4995c677226SJed Brown 5005c677226SJed Brown 5015c677226SJed Brown // Total flux 5025c677226SJed Brown CeedScalar Flux[5][3]; 5033c4b7af6SJed Brown for (CeedInt j=0; j<3; j++) { 5045c677226SJed Brown Flux[0][j] = F_inviscid[j].density; 505ba6664aeSJames Wright for (CeedInt k=0; k<3; k++) 5065c677226SJed Brown Flux[k+1][j] = F_inviscid[j].momentum[k] - stress[k][j]; 5075c677226SJed Brown Flux[4][j] = F_inviscid[j].E_total + Fe[j]; 5085c677226SJed Brown } 5095c677226SJed Brown 5103c4b7af6SJed Brown for (CeedInt j=0; j<3; j++) { 5113c4b7af6SJed Brown for (CeedInt k=0; k<5; k++) { 512a3ae0734SJed Brown Grad_v[j][k][i] = -wdetJ * (dXdx[j][0] * Flux[k][0] + 5135c677226SJed Brown dXdx[j][1] * Flux[k][1] + 5145c677226SJed Brown dXdx[j][2] * Flux[k][2]); 5155c677226SJed Brown } 5165c677226SJed Brown } 5175c677226SJed Brown 5185c677226SJed Brown const CeedScalar body_force[5] = {0, s.U.density *g[0], s.U.density *g[1], s.U.density *g[2], 0}; 5193c4b7af6SJed Brown for (CeedInt j=0; j<5; j++) 5205c677226SJed Brown v[j][i] = wdetJ * (q_dot[j][i] - body_force[j]); 52188b783a1SJames Wright 52288b783a1SJames Wright // jacob_F_conv[3][5][5] = dF(convective)/dq at each direction 5235c677226SJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 5245c677226SJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 5255c677226SJed Brown gamma, g, x_i); 5265c677226SJed Brown CeedScalar grad_U[5][3]; 527ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) { 5285c677226SJed Brown grad_U[0][j] = grad_s[j].U.density; 5293c4b7af6SJed Brown for (CeedInt k=0; k<3; k++) grad_U[k+1][j] = grad_s[j].U.momentum[k]; 5305c677226SJed Brown grad_U[4][j] = grad_s[j].U.E_total; 53188b783a1SJames Wright } 5325c677226SJed Brown 53388b783a1SJames Wright // strong_conv = dF/dq * dq/dx (Strong convection) 53488b783a1SJames Wright CeedScalar strong_conv[5] = {0}; 535ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) 536ba6664aeSJames Wright for (CeedInt k=0; k<5; k++) 537ba6664aeSJames Wright for (CeedInt l=0; l<5; l++) 5385c677226SJed Brown strong_conv[k] += jacob_F_conv[j][k][l] * grad_U[l][j]; 53988b783a1SJames Wright 54088b783a1SJames Wright // Strong residual 54188b783a1SJames Wright CeedScalar strong_res[5]; 542ba6664aeSJames Wright for (CeedInt j=0; j<5; j++) 54388b783a1SJames Wright strong_res[j] = q_dot[j][i] + strong_conv[j] - body_force[j]; 54488b783a1SJames Wright 54588b783a1SJames Wright // -- Stabilization method: none, SU, or SUPG 54688626eedSJames Wright CeedScalar stab[5][3] = {{0.}}; 54788626eedSJames Wright CeedScalar tau_strong_res[5] = {0.}, tau_strong_res_conservative[5] = {0}; 54888626eedSJames Wright CeedScalar tau_strong_conv[5] = {0.}, tau_strong_conv_conservative[5] = {0}; 54988626eedSJames Wright CeedScalar Tau_d[3] = {0.}; 55088b783a1SJames Wright switch (context->stabilization) { 55188b783a1SJames Wright case STAB_NONE: // Galerkin 55288b783a1SJames Wright break; 55388b783a1SJames Wright case STAB_SU: // SU 5545c677226SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 55588626eedSJames Wright tau_strong_conv[0] = Tau_d[0] * strong_conv[0]; 55688626eedSJames Wright tau_strong_conv[1] = Tau_d[1] * strong_conv[1]; 55788626eedSJames Wright tau_strong_conv[2] = Tau_d[1] * strong_conv[2]; 55888626eedSJames Wright tau_strong_conv[3] = Tau_d[1] * strong_conv[3]; 55988626eedSJames Wright tau_strong_conv[4] = Tau_d[2] * strong_conv[4]; 5605c677226SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 5615c677226SJed Brown tau_strong_conv, tau_strong_conv_conservative); 562ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) 563ba6664aeSJames Wright for (CeedInt k=0; k<5; k++) 564ba6664aeSJames Wright for (CeedInt l=0; l<5; l++) 56588626eedSJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_conv_conservative[l]; 56688b783a1SJames Wright 567ba6664aeSJames Wright for (CeedInt j=0; j<5; j++) 568ba6664aeSJames Wright for (CeedInt k=0; k<3; k++) 569a3ae0734SJed Brown Grad_v[k][j][i] += wdetJ*(stab[j][0] * dXdx[k][0] + 57088b783a1SJames Wright stab[j][1] * dXdx[k][1] + 57188b783a1SJames Wright stab[j][2] * dXdx[k][2]); 5723c4b7af6SJed Brown 57388b783a1SJames Wright break; 57488b783a1SJames Wright case STAB_SUPG: // SUPG 5755c677226SJed Brown Tau_diagPrim(Tau_d, dXdx, s.Y.velocity, cv, context, mu, dt, s.U.density); 57688626eedSJames Wright tau_strong_res[0] = Tau_d[0] * strong_res[0]; 57788626eedSJames Wright tau_strong_res[1] = Tau_d[1] * strong_res[1]; 57888626eedSJames Wright tau_strong_res[2] = Tau_d[1] * strong_res[2]; 57988626eedSJames Wright tau_strong_res[3] = Tau_d[1] * strong_res[3]; 58088626eedSJames Wright tau_strong_res[4] = Tau_d[2] * strong_res[4]; 58188626eedSJames Wright // Alternate route (useful later with primitive variable code) 58288626eedSJames Wright // this function was verified against PHASTA for as IC that was as close as possible 58388626eedSJames Wright // computeFluxJacobian_NSp(jacob_F_conv_p, rho, u, E, Rd, cv); 58488626eedSJames Wright // it has also been verified to compute a correct through the following 58588626eedSJames Wright // stab[k][j] += jacob_F_conv_p[j][k][l] * tau_strong_res[l] // flux Jacobian wrt primitive 58688626eedSJames Wright // applied in the triple loop below 58788626eedSJames Wright // However, it is more flops than using the existing Jacobian wrt q after q_{,Y} viz 5885c677226SJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 5895c677226SJed Brown tau_strong_res, tau_strong_res_conservative); 590ba6664aeSJames Wright for (CeedInt j=0; j<3; j++) 591ba6664aeSJames Wright for (CeedInt k=0; k<5; k++) 592ba6664aeSJames Wright for (CeedInt l=0; l<5; l++) 59388626eedSJames Wright stab[k][j] += jacob_F_conv[j][k][l] * tau_strong_res_conservative[l]; 59488b783a1SJames Wright 595ba6664aeSJames Wright for (CeedInt j=0; j<5; j++) 596ba6664aeSJames Wright for (CeedInt k=0; k<3; k++) 597a3ae0734SJed Brown Grad_v[k][j][i] += wdetJ*(stab[j][0] * dXdx[k][0] + 59888b783a1SJames Wright stab[j][1] * dXdx[k][1] + 59988b783a1SJames Wright stab[j][2] * dXdx[k][2]); 60088b783a1SJames Wright break; 60188b783a1SJames Wright } 6023c4b7af6SJed Brown for (CeedInt j=0; j<5; j++) jac_data[j][i] = U[j]; 6033c4b7af6SJed Brown for (CeedInt j=0; j<6; j++) jac_data[5+j][i] = kmstress[j]; 6043c4b7af6SJed Brown for (CeedInt j=0; j<3; j++) jac_data[5+6+j][i] = Tau_d[j]; 60588b783a1SJames Wright 60688b783a1SJames Wright } // End Quadrature Point Loop 60788b783a1SJames Wright 60888b783a1SJames Wright // Return 60988b783a1SJames Wright return 0; 61088b783a1SJames Wright } 611e334ad8fSJed Brown 612e334ad8fSJed Brown CEED_QFUNCTION(IJacobian_Newtonian)(void *ctx, CeedInt Q, 613e334ad8fSJed Brown const CeedScalar *const *in, 614e334ad8fSJed Brown CeedScalar *const *out) { 615e334ad8fSJed Brown // *INDENT-OFF* 616e334ad8fSJed Brown // Inputs 617e334ad8fSJed Brown const CeedScalar (*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 618e334ad8fSJed Brown (*Grad_dq)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 619e334ad8fSJed Brown (*q_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 620e334ad8fSJed Brown (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3], 621e334ad8fSJed Brown (*jac_data)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[4]; 622e334ad8fSJed Brown // Outputs 623e334ad8fSJed Brown CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 624e334ad8fSJed Brown (*Grad_v)[5][CEED_Q_VLA] = (CeedScalar(*)[5][CEED_Q_VLA])out[1]; 625e334ad8fSJed Brown // *INDENT-ON* 626e334ad8fSJed Brown // Context 627e334ad8fSJed Brown NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 628e334ad8fSJed Brown const CeedScalar *g = context->g; 629e334ad8fSJed Brown const CeedScalar cp = context->cp; 630e334ad8fSJed Brown const CeedScalar cv = context->cv; 631e334ad8fSJed Brown const CeedScalar Rd = cp - cv; 632e334ad8fSJed Brown const CeedScalar gamma = cp / cv; 633e334ad8fSJed Brown 634e334ad8fSJed Brown CeedPragmaSIMD 635e334ad8fSJed Brown // Quadrature Point Loop 636e334ad8fSJed Brown for (CeedInt i=0; i<Q; i++) { 637e334ad8fSJed Brown // -- Interp-to-Interp q_data 638e334ad8fSJed Brown const CeedScalar wdetJ = q_data[0][i]; 639e334ad8fSJed Brown // -- Interp-to-Grad q_data 640e334ad8fSJed Brown // ---- Inverse of change of coordinate matrix: X_i,j 641e334ad8fSJed Brown // *INDENT-OFF* 642e334ad8fSJed Brown const CeedScalar dXdx[3][3] = {{q_data[1][i], 643e334ad8fSJed Brown q_data[2][i], 644e334ad8fSJed Brown q_data[3][i]}, 645e334ad8fSJed Brown {q_data[4][i], 646e334ad8fSJed Brown q_data[5][i], 647e334ad8fSJed Brown q_data[6][i]}, 648e334ad8fSJed Brown {q_data[7][i], 649e334ad8fSJed Brown q_data[8][i], 650e334ad8fSJed Brown q_data[9][i]} 651e334ad8fSJed Brown }; 652e334ad8fSJed Brown // *INDENT-ON* 653e334ad8fSJed Brown 654e334ad8fSJed Brown CeedScalar U[5], kmstress[6], Tau_d[3] __attribute((unused)); 655e334ad8fSJed Brown for (int j=0; j<5; j++) U[j] = jac_data[j][i]; 656e334ad8fSJed Brown for (int j=0; j<6; j++) kmstress[j] = jac_data[5+j][i]; 657e334ad8fSJed Brown for (int j=0; j<3; j++) Tau_d[j] = jac_data[5+6+j][i]; 658e334ad8fSJed Brown const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 659e334ad8fSJed Brown State s = StateFromU(context, U, x_i); 660e334ad8fSJed Brown 661e334ad8fSJed Brown CeedScalar dU[5], dx0[3] = {0}; 662e334ad8fSJed Brown for (int j=0; j<5; j++) dU[j] = dq[j][i]; 663e334ad8fSJed Brown State ds = StateFromU_fwd(context, s, dU, x_i, dx0); 664e334ad8fSJed Brown 665e334ad8fSJed Brown State grad_ds[3]; 666e334ad8fSJed Brown for (int j=0; j<3; j++) { 667e334ad8fSJed Brown CeedScalar dUj[5]; 668e334ad8fSJed Brown for (int k=0; k<5; k++) dUj[k] = Grad_dq[0][k][i] * dXdx[0][j] 669e334ad8fSJed Brown + Grad_dq[1][k][i] * dXdx[1][j] 670e334ad8fSJed Brown + Grad_dq[2][k][i] * dXdx[2][j]; 671e334ad8fSJed Brown grad_ds[j] = StateFromU_fwd(context, s, dUj, x_i, dx0); 672e334ad8fSJed Brown } 673e334ad8fSJed Brown 674e334ad8fSJed Brown CeedScalar dstrain_rate[6], dkmstress[6], stress[3][3], dstress[3][3], dFe[3]; 675e334ad8fSJed Brown KMStrainRate(grad_ds, dstrain_rate); 676e334ad8fSJed Brown NewtonianStress(context, dstrain_rate, dkmstress); 677e334ad8fSJed Brown KMUnpack(dkmstress, dstress); 678e334ad8fSJed Brown KMUnpack(kmstress, stress); 679e334ad8fSJed Brown ViscousEnergyFlux_fwd(context, s.Y, ds.Y, grad_ds, stress, dstress, dFe); 680e334ad8fSJed Brown 681e334ad8fSJed Brown StateConservative dF_inviscid[3]; 682e334ad8fSJed Brown FluxInviscid_fwd(context, s, ds, dF_inviscid); 683e334ad8fSJed Brown 684e334ad8fSJed Brown // Total flux 685e334ad8fSJed Brown CeedScalar dFlux[5][3]; 686e334ad8fSJed Brown for (int j=0; j<3; j++) { 687e334ad8fSJed Brown dFlux[0][j] = dF_inviscid[j].density; 688e334ad8fSJed Brown for (int k=0; k<3; k++) 689e334ad8fSJed Brown dFlux[k+1][j] = dF_inviscid[j].momentum[k] - dstress[k][j]; 690e334ad8fSJed Brown dFlux[4][j] = dF_inviscid[j].E_total + dFe[j]; 691e334ad8fSJed Brown } 692e334ad8fSJed Brown 693e334ad8fSJed Brown for (int j=0; j<3; j++) { 694e334ad8fSJed Brown for (int k=0; k<5; k++) { 695e334ad8fSJed Brown Grad_v[j][k][i] = -wdetJ * (dXdx[j][0] * dFlux[k][0] + 696e334ad8fSJed Brown dXdx[j][1] * dFlux[k][1] + 697e334ad8fSJed Brown dXdx[j][2] * dFlux[k][2]); 698e334ad8fSJed Brown } 699e334ad8fSJed Brown } 700e334ad8fSJed Brown 701e334ad8fSJed Brown const CeedScalar dbody_force[5] = {0, ds.U.density *g[0], ds.U.density *g[1], ds.U.density *g[2], 0}; 702e334ad8fSJed Brown for (int j=0; j<5; j++) 703e334ad8fSJed Brown v[j][i] = wdetJ * (context->ijacobian_time_shift * dU[j] - dbody_force[j]); 704e334ad8fSJed Brown 705e334ad8fSJed Brown if (1) { 706e334ad8fSJed Brown CeedScalar jacob_F_conv[3][5][5] = {0}; 707e334ad8fSJed Brown computeFluxJacobian_NS(jacob_F_conv, s.U.density, s.Y.velocity, s.U.E_total, 708e334ad8fSJed Brown gamma, g, x_i); 709e334ad8fSJed Brown CeedScalar grad_dU[5][3]; 710e334ad8fSJed Brown for (int j=0; j<3; j++) { 711e334ad8fSJed Brown grad_dU[0][j] = grad_ds[j].U.density; 712e334ad8fSJed Brown for (int k=0; k<3; k++) grad_dU[k+1][j] = grad_ds[j].U.momentum[k]; 713e334ad8fSJed Brown grad_dU[4][j] = grad_ds[j].U.E_total; 714e334ad8fSJed Brown } 715e334ad8fSJed Brown CeedScalar dstrong_conv[5] = {0}; 716e334ad8fSJed Brown for (int j=0; j<3; j++) 717e334ad8fSJed Brown for (int k=0; k<5; k++) 718e334ad8fSJed Brown for (int l=0; l<5; l++) 719e334ad8fSJed Brown dstrong_conv[k] += jacob_F_conv[j][k][l] * grad_dU[l][j]; 720e334ad8fSJed Brown CeedScalar dstrong_res[5]; 721e334ad8fSJed Brown for (int j=0; j<5; j++) 722e334ad8fSJed Brown dstrong_res[j] = context->ijacobian_time_shift * dU[j] + dstrong_conv[j] - 723e334ad8fSJed Brown dbody_force[j]; 724e334ad8fSJed Brown CeedScalar dtau_strong_res[5] = {0.}, dtau_strong_res_conservative[5] = {0}; 725e334ad8fSJed Brown dtau_strong_res[0] = Tau_d[0] * dstrong_res[0]; 726e334ad8fSJed Brown dtau_strong_res[1] = Tau_d[1] * dstrong_res[1]; 727e334ad8fSJed Brown dtau_strong_res[2] = Tau_d[1] * dstrong_res[2]; 728e334ad8fSJed Brown dtau_strong_res[3] = Tau_d[1] * dstrong_res[3]; 729e334ad8fSJed Brown dtau_strong_res[4] = Tau_d[2] * dstrong_res[4]; 730e334ad8fSJed Brown PrimitiveToConservative_fwd(s.U.density, s.Y.velocity, s.U.E_total, Rd, cv, 731e334ad8fSJed Brown dtau_strong_res, dtau_strong_res_conservative); 732e334ad8fSJed Brown CeedScalar dstab[5][3] = {0}; 733e334ad8fSJed Brown for (int j=0; j<3; j++) 734e334ad8fSJed Brown for (int k=0; k<5; k++) 735e334ad8fSJed Brown for (int l=0; l<5; l++) 736e334ad8fSJed Brown dstab[k][j] += jacob_F_conv[j][k][l] * dtau_strong_res_conservative[l]; 737e334ad8fSJed Brown for (int j=0; j<5; j++) 738e334ad8fSJed Brown for (int k=0; k<3; k++) 739e334ad8fSJed Brown Grad_v[k][j][i] += wdetJ*(dstab[j][0] * dXdx[k][0] + 740e334ad8fSJed Brown dstab[j][1] * dXdx[k][1] + 741e334ad8fSJed Brown dstab[j][2] * dXdx[k][2]); 742e334ad8fSJed Brown 743e334ad8fSJed Brown } 744e334ad8fSJed Brown } // End Quadrature Point Loop 745e334ad8fSJed Brown return 0; 746e334ad8fSJed Brown } 74765dd5cafSJames Wright 74865dd5cafSJames Wright // Compute boundary integral (ie. for strongly set inflows) 74965dd5cafSJames Wright CEED_QFUNCTION(BoundaryIntegral)(void *ctx, CeedInt Q, 75065dd5cafSJames Wright const CeedScalar *const *in, 75165dd5cafSJames Wright CeedScalar *const *out) { 75265dd5cafSJames Wright 75365dd5cafSJames Wright //*INDENT-OFF* 75465dd5cafSJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 755*2c4e60d7SJames Wright (*Grad_q)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 756*2c4e60d7SJames Wright (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 757*2c4e60d7SJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 75865dd5cafSJames Wright 75965dd5cafSJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA]) out[0]; 76065dd5cafSJames Wright 76165dd5cafSJames Wright //*INDENT-ON* 76265dd5cafSJames Wright 763*2c4e60d7SJames Wright const NewtonianIdealGasContext context = (NewtonianIdealGasContext) ctx; 764*2c4e60d7SJames Wright const bool is_implicit = context->is_implicit; 76565dd5cafSJames Wright 76665dd5cafSJames Wright CeedPragmaSIMD 76765dd5cafSJames Wright for(CeedInt i=0; i<Q; i++) { 768*2c4e60d7SJames Wright const CeedScalar U[5] = {q[0][i], q[1][i], q[2][i], q[3][i], q[4][i]}; 769*2c4e60d7SJames Wright const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 770*2c4e60d7SJames Wright const State s = StateFromU(context, U, x_i); 77165dd5cafSJames Wright 77265dd5cafSJames Wright const CeedScalar wdetJb = (is_implicit ? -1. : 1.) * q_data_sur[0][i]; 77365dd5cafSJames Wright // ---- Normal vect 77465dd5cafSJames Wright const CeedScalar norm[3] = {q_data_sur[1][i], 77565dd5cafSJames Wright q_data_sur[2][i], 77665dd5cafSJames Wright q_data_sur[3][i] 77765dd5cafSJames Wright }; 77865dd5cafSJames Wright 779*2c4e60d7SJames Wright const CeedScalar dXdx[2][3] = { 780*2c4e60d7SJames Wright {q_data_sur[4][i], q_data_sur[5][i], q_data_sur[6][i]}, 781*2c4e60d7SJames Wright {q_data_sur[7][i], q_data_sur[8][i], q_data_sur[9][i]} 782*2c4e60d7SJames Wright }; 78365dd5cafSJames Wright 784*2c4e60d7SJames Wright State grad_s[3]; 785*2c4e60d7SJames Wright for (CeedInt j=0; j<3; j++) { 786*2c4e60d7SJames Wright CeedScalar dx_i[3] = {0}, dU[5]; 787*2c4e60d7SJames Wright for (CeedInt k=0; k<5; k++) 788*2c4e60d7SJames Wright dU[k] = Grad_q[0][k][i] * dXdx[0][j] + 789*2c4e60d7SJames Wright Grad_q[1][k][i] * dXdx[1][j]; 790*2c4e60d7SJames Wright dx_i[j] = 1.; 791*2c4e60d7SJames Wright grad_s[j] = StateFromU_fwd(context, s, dU, x_i, dx_i); 792*2c4e60d7SJames Wright } 79365dd5cafSJames Wright 794*2c4e60d7SJames Wright CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 795*2c4e60d7SJames Wright KMStrainRate(grad_s, strain_rate); 796*2c4e60d7SJames Wright NewtonianStress(context, strain_rate, kmstress); 797*2c4e60d7SJames Wright KMUnpack(kmstress, stress); 798*2c4e60d7SJames Wright ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 799*2c4e60d7SJames Wright 800*2c4e60d7SJames Wright StateConservative F_inviscid[3]; 801*2c4e60d7SJames Wright FluxInviscid(context, s, F_inviscid); 802*2c4e60d7SJames Wright 803*2c4e60d7SJames Wright CeedScalar Flux[5] = {0.}; 804*2c4e60d7SJames Wright for (int j=0; j<3; j++) { 805*2c4e60d7SJames Wright Flux[0] += F_inviscid[j].density * norm[j]; 806*2c4e60d7SJames Wright for (int k=0; k<3; k++) 807*2c4e60d7SJames Wright Flux[k+1] += (F_inviscid[j].momentum[k] - stress[k][j]) * norm[j]; 808*2c4e60d7SJames Wright Flux[4] += (F_inviscid[j].E_total + Fe[j])*norm[j]; 809*2c4e60d7SJames Wright } 810*2c4e60d7SJames Wright 81165dd5cafSJames Wright // -- Density 812*2c4e60d7SJames Wright v[0][i] = -wdetJb * Flux[0]; 81365dd5cafSJames Wright 81465dd5cafSJames Wright // -- Momentum 81565dd5cafSJames Wright for (CeedInt j=0; j<3; j++) 816*2c4e60d7SJames Wright v[j+1][i] = -wdetJb * Flux[j+1]; 81765dd5cafSJames Wright 81865dd5cafSJames Wright // -- Total Energy Density 819*2c4e60d7SJames Wright v[4][i] = -wdetJb * Flux[4]; 82065dd5cafSJames Wright } 82165dd5cafSJames Wright return 0; 82265dd5cafSJames Wright } 82365dd5cafSJames Wright 82430e9fa81SJames Wright // Outflow boundary condition, weakly setting a constant pressure 82530e9fa81SJames Wright CEED_QFUNCTION(PressureOutflow)(void *ctx, CeedInt Q, 82630e9fa81SJames Wright const CeedScalar *const *in, 82730e9fa81SJames Wright CeedScalar *const *out) { 82830e9fa81SJames Wright // *INDENT-OFF* 82930e9fa81SJames Wright // Inputs 83030e9fa81SJames Wright const CeedScalar (*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 831ce9b5c20SJames Wright (*Grad_q)[5][CEED_Q_VLA] = (const CeedScalar(*)[5][CEED_Q_VLA])in[1], 832ce9b5c20SJames Wright (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2], 833ce9b5c20SJames Wright (*x)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3]; 83430e9fa81SJames Wright // Outputs 83530e9fa81SJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0], 83630e9fa81SJames Wright (*jac_data_sur)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[1]; 83730e9fa81SJames Wright // *INDENT-ON* 83830e9fa81SJames Wright 83930e9fa81SJames Wright const NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 84030e9fa81SJames Wright const bool implicit = context->is_implicit; 84130e9fa81SJames Wright const CeedScalar P0 = context->P0; 84230e9fa81SJames Wright 84330e9fa81SJames Wright CeedPragmaSIMD 84430e9fa81SJames Wright // Quadrature Point Loop 84530e9fa81SJames Wright for (CeedInt i=0; i<Q; i++) { 84630e9fa81SJames Wright // Setup 84730e9fa81SJames Wright // -- Interp in 848ce9b5c20SJames Wright const CeedScalar U[5] = {q[0][i], q[1][i], q[2][i], q[3][i], q[4][i]}; 849ce9b5c20SJames Wright const CeedScalar x_i[3] = {x[0][i], x[1][i], x[2][i]}; 850ce9b5c20SJames Wright State s = StateFromU(context, U, x_i); 851ce9b5c20SJames Wright s.Y.pressure = P0; 85230e9fa81SJames Wright 85330e9fa81SJames Wright // -- Interp-to-Interp q_data 85430e9fa81SJames Wright // For explicit mode, the surface integral is on the RHS of ODE q_dot = f(q). 85530e9fa81SJames Wright // For implicit mode, it gets pulled to the LHS of implicit ODE/DAE g(q_dot, q). 85630e9fa81SJames Wright // We can effect this by swapping the sign on this weight 85730e9fa81SJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 85830e9fa81SJames Wright 85930e9fa81SJames Wright // ---- Normal vect 86030e9fa81SJames Wright const CeedScalar norm[3] = {q_data_sur[1][i], 86130e9fa81SJames Wright q_data_sur[2][i], 86230e9fa81SJames Wright q_data_sur[3][i] 86330e9fa81SJames Wright }; 86430e9fa81SJames Wright 865ce9b5c20SJames Wright const CeedScalar dXdx[2][3] = { 866ce9b5c20SJames Wright {q_data_sur[4][i], q_data_sur[5][i], q_data_sur[6][i]}, 867ce9b5c20SJames Wright {q_data_sur[7][i], q_data_sur[8][i], q_data_sur[9][i]} 868ce9b5c20SJames Wright }; 86930e9fa81SJames Wright 870ce9b5c20SJames Wright State grad_s[3]; 871ce9b5c20SJames Wright for (CeedInt j=0; j<3; j++) { 872ce9b5c20SJames Wright CeedScalar dx_i[3] = {0}, dU[5]; 873ce9b5c20SJames Wright for (CeedInt k=0; k<5; k++) 874ce9b5c20SJames Wright dU[k] = Grad_q[0][k][i] * dXdx[0][j] + 875ce9b5c20SJames Wright Grad_q[1][k][i] * dXdx[1][j]; 876ce9b5c20SJames Wright dx_i[j] = 1.; 877ce9b5c20SJames Wright grad_s[j] = StateFromU_fwd(context, s, dU, x_i, dx_i); 878ce9b5c20SJames Wright } 879ce9b5c20SJames Wright 880ce9b5c20SJames Wright CeedScalar strain_rate[6], kmstress[6], stress[3][3], Fe[3]; 881ce9b5c20SJames Wright KMStrainRate(grad_s, strain_rate); 882ce9b5c20SJames Wright NewtonianStress(context, strain_rate, kmstress); 883ce9b5c20SJames Wright KMUnpack(kmstress, stress); 884ce9b5c20SJames Wright ViscousEnergyFlux(context, s.Y, grad_s, stress, Fe); 885ce9b5c20SJames Wright 886ce9b5c20SJames Wright StateConservative F_inviscid[3]; 887ce9b5c20SJames Wright FluxInviscid(context, s, F_inviscid); 888ce9b5c20SJames Wright 889ce9b5c20SJames Wright CeedScalar Flux[5] = {0.}; 890ce9b5c20SJames Wright for (int j=0; j<3; j++) { 891ce9b5c20SJames Wright Flux[0] += F_inviscid[j].density * norm[j]; 892ce9b5c20SJames Wright for (int k=0; k<3; k++) 893ce9b5c20SJames Wright Flux[k+1] += (F_inviscid[j].momentum[k] - stress[k][j]) * norm[j]; 894ce9b5c20SJames Wright Flux[4] += (F_inviscid[j].E_total + Fe[j])*norm[j]; 895ce9b5c20SJames Wright } 89630e9fa81SJames Wright 89730e9fa81SJames Wright // -- Density 898ce9b5c20SJames Wright v[0][i] = -wdetJb * Flux[0]; 89930e9fa81SJames Wright 90030e9fa81SJames Wright // -- Momentum 90130e9fa81SJames Wright for (CeedInt j=0; j<3; j++) 902ce9b5c20SJames Wright v[j+1][i] = -wdetJb * Flux[j+1]; 90330e9fa81SJames Wright 90430e9fa81SJames Wright // -- Total Energy Density 905ce9b5c20SJames Wright v[4][i] = -wdetJb * Flux[4]; 90630e9fa81SJames Wright 90730e9fa81SJames Wright // Save values for Jacobian 908ce9b5c20SJames Wright jac_data_sur[0][i] = s.U.density; 909ce9b5c20SJames Wright jac_data_sur[1][i] = s.Y.velocity[0]; 910ce9b5c20SJames Wright jac_data_sur[2][i] = s.Y.velocity[1]; 911ce9b5c20SJames Wright jac_data_sur[3][i] = s.Y.velocity[2]; 912ce9b5c20SJames Wright jac_data_sur[4][i] = s.U.E_total; 91330e9fa81SJames Wright } // End Quadrature Point Loop 91430e9fa81SJames Wright return 0; 91530e9fa81SJames Wright } 91630e9fa81SJames Wright 91730e9fa81SJames Wright // Jacobian for weak-pressure outflow boundary condition 91830e9fa81SJames Wright CEED_QFUNCTION(PressureOutflow_Jacobian)(void *ctx, CeedInt Q, 91930e9fa81SJames Wright const CeedScalar *const *in, 92030e9fa81SJames Wright CeedScalar *const *out) { 92130e9fa81SJames Wright // *INDENT-OFF* 92230e9fa81SJames Wright // Inputs 92330e9fa81SJames Wright const CeedScalar (*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0], 92430e9fa81SJames Wright (*q_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[1], 92530e9fa81SJames Wright (*jac_data_sur)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[2]; 92630e9fa81SJames Wright // Outputs 92730e9fa81SJames Wright CeedScalar (*v)[CEED_Q_VLA] = (CeedScalar(*)[CEED_Q_VLA])out[0]; 92830e9fa81SJames Wright // *INDENT-ON* 92930e9fa81SJames Wright 93030e9fa81SJames Wright const NewtonianIdealGasContext context = (NewtonianIdealGasContext)ctx; 93130e9fa81SJames Wright const bool implicit = context->is_implicit; 93230e9fa81SJames Wright 93330e9fa81SJames Wright CeedPragmaSIMD 93430e9fa81SJames Wright // Quadrature Point Loop 93530e9fa81SJames Wright for (CeedInt i=0; i<Q; i++) { 93630e9fa81SJames Wright const CeedScalar rho = jac_data_sur[0][i]; 93730e9fa81SJames Wright const CeedScalar u[3] = {jac_data_sur[1][i], jac_data_sur[2][i], jac_data_sur[3][i]}; 93830e9fa81SJames Wright const CeedScalar E = jac_data_sur[4][i]; 93930e9fa81SJames Wright 94030e9fa81SJames Wright const CeedScalar drho = dq[0][i]; 94130e9fa81SJames Wright const CeedScalar dmomentum[3] = {dq[1][i], dq[2][i], dq[3][i]}; 94230e9fa81SJames Wright const CeedScalar dE = dq[4][i]; 94330e9fa81SJames Wright 94430e9fa81SJames Wright const CeedScalar wdetJb = (implicit ? -1. : 1.) * q_data_sur[0][i]; 94530e9fa81SJames Wright const CeedScalar norm[3] = {q_data_sur[1][i], 94630e9fa81SJames Wright q_data_sur[2][i], 94730e9fa81SJames Wright q_data_sur[3][i] 94830e9fa81SJames Wright }; 94930e9fa81SJames Wright 95030e9fa81SJames Wright CeedScalar du[3]; 95130e9fa81SJames Wright for (int j=0; j<3; j++) du[j] = (dmomentum[j] - u[j] * drho) / rho; 95230e9fa81SJames Wright const CeedScalar u_normal = Dot3(norm, u); 95330e9fa81SJames Wright const CeedScalar du_normal = Dot3(norm, du); 95430e9fa81SJames Wright const CeedScalar dmomentum_normal = drho * u_normal + rho * du_normal; 95530e9fa81SJames Wright const CeedScalar P = context->P0; 95630e9fa81SJames Wright const CeedScalar dP = 0; 95730e9fa81SJames Wright 95830e9fa81SJames Wright v[0][i] = -wdetJb * dmomentum_normal; 95930e9fa81SJames Wright for (int j=0; j<3; j++) 96030e9fa81SJames Wright v[j+1][i] = -wdetJb * (dmomentum_normal * u[j] + rho * u_normal * du[j]); 96130e9fa81SJames Wright v[4][i] = -wdetJb * (du_normal * (E + P) + u_normal * (dE + dP)); 96230e9fa81SJames Wright } // End Quadrature Point Loop 96330e9fa81SJames Wright return 0; 96430e9fa81SJames Wright } 96530e9fa81SJames Wright 96688b783a1SJames Wright // ***************************************************************************** 96788b783a1SJames Wright #endif // newtonian_h 968