xref: /honee/qfunctions/blasius.h (revision 512c8ec7bf287932c614112e0f1147c31168267a)
1dc936754SJeremy L Thompson // Copyright (c) 2017-2024, Lawrence Livermore National Security, LLC and other CEED contributors.
2bb8a0c61SJames Wright // All Rights Reserved. See the top-level LICENSE and NOTICE files for details.
3bb8a0c61SJames Wright //
4bb8a0c61SJames Wright // SPDX-License-Identifier: BSD-2-Clause
5bb8a0c61SJames Wright //
6bb8a0c61SJames Wright // This file is part of CEED:  http://github.com/ceed
7bb8a0c61SJames Wright 
8bb8a0c61SJames Wright /// @file
9bb8a0c61SJames Wright /// Operator for Navier-Stokes example using PETSc
10bb8a0c61SJames Wright #include <ceed.h>
112b916ea7SJeremy L Thompson 
12e0d1a4dfSLeila Ghaffari #include "newtonian_state.h"
1315a3537eSJed Brown #include "newtonian_types.h"
14704b8bbeSJames Wright #include "utils.h"
15bb8a0c61SJames Wright 
160d850f2eSLeila Ghaffari #define BLASIUS_MAX_N_CHEBYSHEV 50
170d850f2eSLeila Ghaffari 
18bb8a0c61SJames Wright typedef struct BlasiusContext_ *BlasiusContext;
19bb8a0c61SJames Wright struct BlasiusContext_ {
20bb8a0c61SJames Wright   bool                             implicit;                              // !< Using implicit timesteping or not
212acc7cbcSKenneth E. Jansen   bool                             weakT;                                 // !< flag to set Temperature weakly at inflow
22bb8a0c61SJames Wright   CeedScalar                       delta0;                                // !< Boundary layer height at inflow
23aef1eb53SLeila Ghaffari   CeedScalar                       U_inf;                                 // !< Velocity at boundary layer edge
24aef1eb53SLeila Ghaffari   CeedScalar                       T_inf;                                 // !< Temperature at boundary layer edge
25e0d1a4dfSLeila Ghaffari   CeedScalar                       T_wall;                                // !< Temperature at the wall
26bb8a0c61SJames Wright   CeedScalar                       P0;                                    // !< Pressure at outflow
27ef2c71fdSJames Wright   CeedScalar                       x_inflow;                              // !< Location of inflow in x
28e0d1a4dfSLeila Ghaffari   CeedScalar                       n_cheb;                                // !< Number of Chebyshev terms
290d850f2eSLeila Ghaffari   CeedScalar                      *X;                                     // !< Chebyshev polynomial coordinate vector (CPU only)
30e0d1a4dfSLeila Ghaffari   CeedScalar                       eta_max;                               // !< Maximum eta in the domain
310d850f2eSLeila Ghaffari   CeedScalar                       Tf_cheb[BLASIUS_MAX_N_CHEBYSHEV];      // !< Chebyshev coefficient for f
320d850f2eSLeila Ghaffari   CeedScalar                       Th_cheb[BLASIUS_MAX_N_CHEBYSHEV - 1];  // !< Chebyshev coefficient for h
33bb8a0c61SJames Wright   struct NewtonianIdealGasContext_ newtonian_ctx;
34bb8a0c61SJames Wright };
35bb8a0c61SJames Wright 
36e0d1a4dfSLeila Ghaffari // *****************************************************************************
3704e40bb6SJeremy L Thompson // This helper function evaluates Chebyshev polynomials with a set of coefficients with all their derivatives represented as a recurrence table.
38e0d1a4dfSLeila Ghaffari // *****************************************************************************
392b916ea7SJeremy L Thompson CEED_QFUNCTION_HELPER void ChebyshevEval(int N, const double *Tf, double x, double eta_max, double *f) {
40e0d1a4dfSLeila Ghaffari   double dX_deta     = 2 / eta_max;
41e0d1a4dfSLeila Ghaffari   double table[4][3] = {
42e0d1a4dfSLeila Ghaffari   // Chebyshev polynomials T_0, T_1, T_2 of the first kind in (-1,1)
432b916ea7SJeremy L Thompson       {1, x, 2 * x * x - 1},
442b916ea7SJeremy L Thompson       {0, 1, 4 * x        },
452b916ea7SJeremy L Thompson       {0, 0, 4            },
462b916ea7SJeremy L Thompson       {0, 0, 0            }
47e0d1a4dfSLeila Ghaffari   };
48e0d1a4dfSLeila Ghaffari   for (int i = 0; i < 4; i++) {
49e0d1a4dfSLeila Ghaffari     // i-th derivative of f
50e0d1a4dfSLeila Ghaffari     f[i] = table[i][0] * Tf[0] + table[i][1] * Tf[1] + table[i][2] * Tf[2];
51e0d1a4dfSLeila Ghaffari   }
52e0d1a4dfSLeila Ghaffari   for (int i = 3; i < N; i++) {
53e0d1a4dfSLeila Ghaffari     // T_n(x) = 2xT_{n-1}(x) - T_{n-2}(x)
54e0d1a4dfSLeila Ghaffari     table[0][i % 3] = 2 * x * table[0][(i - 1) % 3] - table[0][(i - 2) % 3];
55e0d1a4dfSLeila Ghaffari     // Differentiate Chebyshev polynomials with the recurrence relation
56e0d1a4dfSLeila Ghaffari     for (int j = 1; j < 4; j++) {
57e0d1a4dfSLeila Ghaffari       // T'_{n}(x)/n = 2T_{n-1}(x) + T'_{n-2}(x)/n-2
58e0d1a4dfSLeila Ghaffari       table[j][i % 3] = i * (2 * table[j - 1][(i - 1) % 3] + table[j][(i - 2) % 3] / (i - 2));
59e0d1a4dfSLeila Ghaffari     }
60e0d1a4dfSLeila Ghaffari     for (int j = 0; j < 4; j++) {
61e0d1a4dfSLeila Ghaffari       f[j] += table[j][i % 3] * Tf[i];
62bb8a0c61SJames Wright     }
63bb8a0c61SJames Wright   }
64e0d1a4dfSLeila Ghaffari   for (int i = 1; i < 4; i++) {
65e0d1a4dfSLeila Ghaffari     // Transform derivatives from Chebyshev [-1, 1] to [0, eta_max].
66e0d1a4dfSLeila Ghaffari     for (int j = 0; j < i; j++) f[i] *= dX_deta;
67e0d1a4dfSLeila Ghaffari   }
68bb8a0c61SJames Wright }
69bb8a0c61SJames Wright 
70e0d1a4dfSLeila Ghaffari // *****************************************************************************
71e0d1a4dfSLeila Ghaffari // This helper function computes the Blasius boundary layer solution.
72e0d1a4dfSLeila Ghaffari // *****************************************************************************
732b916ea7SJeremy L Thompson State CEED_QFUNCTION_HELPER(BlasiusSolution)(const BlasiusContext blasius, const CeedScalar x[3], const CeedScalar x0, const CeedScalar x_inflow,
740d850f2eSLeila Ghaffari                                              const CeedScalar rho_infty, CeedScalar *t12) {
75e0d1a4dfSLeila Ghaffari   CeedInt    N     = blasius->n_cheb;
760d850f2eSLeila Ghaffari   CeedScalar mu    = blasius->newtonian_ctx.mu;
770d850f2eSLeila Ghaffari   CeedScalar nu    = mu / rho_infty;
78aef1eb53SLeila Ghaffari   CeedScalar eta   = x[1] * sqrt(blasius->U_inf / (nu * (x0 + x[0] - x_inflow)));
79e0d1a4dfSLeila Ghaffari   CeedScalar X     = 2 * (eta / blasius->eta_max) - 1.;
80aef1eb53SLeila Ghaffari   CeedScalar U_inf = blasius->U_inf;
81e0d1a4dfSLeila Ghaffari   CeedScalar Rd    = GasConstant(&blasius->newtonian_ctx);
82e0d1a4dfSLeila Ghaffari 
83e0d1a4dfSLeila Ghaffari   CeedScalar f[4], h[4];
84e0d1a4dfSLeila Ghaffari   ChebyshevEval(N, blasius->Tf_cheb, X, blasius->eta_max, f);
85e0d1a4dfSLeila Ghaffari   ChebyshevEval(N - 1, blasius->Th_cheb, X, blasius->eta_max, h);
86e0d1a4dfSLeila Ghaffari 
870d850f2eSLeila Ghaffari   *t12 = mu * U_inf * f[2] * sqrt(U_inf / (nu * (x0 + x[0] - x_inflow)));
88e0d1a4dfSLeila Ghaffari 
89e0d1a4dfSLeila Ghaffari   CeedScalar Y[5];
90aef1eb53SLeila Ghaffari   Y[1] = U_inf * f[1];
91aef1eb53SLeila Ghaffari   Y[2] = 0.5 * sqrt(nu * U_inf / (x0 + x[0] - x_inflow)) * (eta * f[1] - f[0]);
92e0d1a4dfSLeila Ghaffari   Y[3] = 0.;
93aef1eb53SLeila Ghaffari   Y[4] = blasius->T_inf * h[0];
940d850f2eSLeila Ghaffari   Y[0] = rho_infty / h[0] * Rd * Y[4];
95edcfef1bSKenneth E. Jansen   return StateFromY(&blasius->newtonian_ctx, Y);
96bb8a0c61SJames Wright }
97bb8a0c61SJames Wright 
98bb8a0c61SJames Wright // *****************************************************************************
99bb8a0c61SJames Wright // This QFunction sets a Blasius boundary layer for the initial condition
100bb8a0c61SJames Wright // *****************************************************************************
1012b916ea7SJeremy L Thompson CEED_QFUNCTION(ICsBlasius)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) {
102bb8a0c61SJames Wright   const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0];
103bb8a0c61SJames Wright   CeedScalar(*q0)[CEED_Q_VLA]      = (CeedScalar(*)[CEED_Q_VLA])out[0];
104bb8a0c61SJames Wright 
105bb8a0c61SJames Wright   const BlasiusContext           context  = (BlasiusContext)ctx;
10633796533SJames Wright   const NewtonianIdealGasContext gas      = &context->newtonian_ctx;
107bb8a0c61SJames Wright   const CeedScalar               mu       = context->newtonian_ctx.mu;
108bb8a0c61SJames Wright   const CeedScalar               delta0   = context->delta0;
109ef2c71fdSJames Wright   const CeedScalar               x_inflow = context->x_inflow;
110e0d1a4dfSLeila Ghaffari   CeedScalar                     t12;
111bb8a0c61SJames Wright 
11233796533SJames Wright   const CeedScalar Y_inf[5] = {context->P0, context->U_inf, 0, 0, context->T_inf};
113edcfef1bSKenneth E. Jansen   const State      s_inf    = StateFromY(gas, Y_inf);
114bb8a0c61SJames Wright 
11533796533SJames Wright   const CeedScalar x0 = context->U_inf * s_inf.U.density / (mu * 25 / Square(delta0));
11633796533SJames Wright 
11733796533SJames Wright   CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) {
11833796533SJames Wright     const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]};
11933796533SJames Wright     State            s    = BlasiusSolution(context, x, x0, x_inflow, s_inf.U.density, &t12);
12033796533SJames Wright     CeedScalar       q[5] = {0};
12133796533SJames Wright 
12233796533SJames Wright     switch (gas->state_var) {
12333796533SJames Wright       case STATEVAR_CONSERVATIVE:
12433796533SJames Wright         UnpackState_U(s.U, q);
12533796533SJames Wright         break;
12633796533SJames Wright       case STATEVAR_PRIMITIVE:
12733796533SJames Wright         UnpackState_Y(s.Y, q);
12833796533SJames Wright         break;
12933796533SJames Wright     }
13033796533SJames Wright     for (CeedInt j = 0; j < 5; j++) q0[j][i] = q[j];
13133796533SJames Wright   }
132bb8a0c61SJames Wright   return 0;
133bb8a0c61SJames Wright }
134bb8a0c61SJames Wright 
135bb8a0c61SJames Wright // *****************************************************************************
1362b916ea7SJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) {
1374b96a86bSJames Wright   const BlasiusContext context     = (BlasiusContext)ctx;
1383d65b166SJames Wright   const CeedScalar(*q)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0];
139ade49511SJames Wright   const CeedScalar(*q_data_sur)    = in[2];
1403d65b166SJames Wright   const CeedScalar(*X)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[3];
141bb8a0c61SJames Wright   CeedScalar(*v)[CEED_Q_VLA]       = (CeedScalar(*)[CEED_Q_VLA])out[0];
1424b96a86bSJames Wright   CeedScalar(*jac_data_sur)        = context->newtonian_ctx.is_implicit ? out[1] : NULL;
1433d65b166SJames Wright 
144ade49511SJames Wright   const bool                     is_implicit = context->implicit;
145*512c8ec7SJames Wright   const NewtonianIdealGasContext gas         = &context->newtonian_ctx;
146*512c8ec7SJames Wright   const CeedScalar               rho_0       = context->P0 / (GasConstant(gas) * context->T_inf);
147*512c8ec7SJames Wright   const CeedScalar               x0          = context->U_inf * rho_0 / (gas->mu * 25 / Square(context->delta0));
14880f5d3cbSJames Wright   const CeedScalar               zeros[11]   = {0.};
149bb8a0c61SJames Wright 
1503d65b166SJames Wright   CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) {
151ade49511SJames Wright     CeedScalar wdetJb, norm[3];
152ade49511SJames Wright     QdataBoundaryUnpack_3D(Q, i, q_data_sur, &wdetJb, NULL, norm);
153ade49511SJames Wright     wdetJb *= is_implicit ? -1. : 1.;
154bb8a0c61SJames Wright 
1552acc7cbcSKenneth E. Jansen     // Calculate inflow values
156e0d1a4dfSLeila Ghaffari     const CeedScalar x[3] = {X[0][i], X[1][i], 0.};
157bb8a0c61SJames Wright     CeedScalar       t12;
158*512c8ec7SJames Wright     State            s = BlasiusSolution(context, x, x0, context->x_inflow, rho_0, &t12);
1590d850f2eSLeila Ghaffari     CeedScalar       qi[5];
1600d850f2eSLeila Ghaffari     for (CeedInt j = 0; j < 5; j++) qi[j] = q[j][i];
161edcfef1bSKenneth E. Jansen     State s_int = StateFromU(gas, qi);
162bb8a0c61SJames Wright 
1632acc7cbcSKenneth E. Jansen     // enabling user to choose between weak T and weak rho inflow
164*512c8ec7SJames Wright     if (context->weakT) {  // density from the current solution
1650d850f2eSLeila Ghaffari       s.U.density = s_int.U.density;
166edcfef1bSKenneth E. Jansen       s.Y         = StatePrimitiveFromConservative(gas, s.U);
1670d850f2eSLeila Ghaffari     } else {  // Total energy from current solution
1680d850f2eSLeila Ghaffari       s.U.E_total = s_int.U.E_total;
169edcfef1bSKenneth E. Jansen       s.Y         = StatePrimitiveFromConservative(gas, s.U);
1702acc7cbcSKenneth E. Jansen     }
1710d850f2eSLeila Ghaffari 
1720d850f2eSLeila Ghaffari     StateConservative Flux_inviscid[3];
1730d850f2eSLeila Ghaffari     FluxInviscid(&context->newtonian_ctx, s, Flux_inviscid);
174bb8a0c61SJames Wright 
1752b916ea7SJeremy L Thompson     const CeedScalar stress[3][3] = {
1762b916ea7SJeremy L Thompson         {0,   t12, 0},
1772b916ea7SJeremy L Thompson         {t12, 0,   0},
1782b916ea7SJeremy L Thompson         {0,   0,   0}
1792b916ea7SJeremy L Thompson     };
1800d850f2eSLeila Ghaffari     const CeedScalar Fe[3] = {0};  // TODO: viscous energy flux needs grad temperature
1810d850f2eSLeila Ghaffari     CeedScalar       Flux[5];
1820d850f2eSLeila Ghaffari     FluxTotal_Boundary(Flux_inviscid, stress, Fe, norm, Flux);
1832b916ea7SJeremy L Thompson     for (CeedInt j = 0; j < 5; j++) v[j][i] = -wdetJb * Flux[j];
1844b96a86bSJames Wright     if (is_implicit) StoredValuesPack(Q, i, 0, 11, zeros, jac_data_sur);
185ade49511SJames Wright   }
186bb8a0c61SJames Wright   return 0;
187bb8a0c61SJames Wright }
188bb8a0c61SJames Wright 
189e0d1a4dfSLeila Ghaffari // *****************************************************************************
1902b916ea7SJeremy L Thompson CEED_QFUNCTION(Blasius_Inflow_Jacobian)(void *ctx, CeedInt Q, const CeedScalar *const *in, CeedScalar *const *out) {
1913d65b166SJames Wright   const CeedScalar(*dq)[CEED_Q_VLA] = (const CeedScalar(*)[CEED_Q_VLA])in[0];
192ade49511SJames Wright   const CeedScalar(*q_data_sur)     = in[2];
1933d65b166SJames Wright   const CeedScalar(*X)[CEED_Q_VLA]  = (const CeedScalar(*)[CEED_Q_VLA])in[3];
194f0b65372SJed Brown   CeedScalar(*v)[CEED_Q_VLA]        = (CeedScalar(*)[CEED_Q_VLA])out[0];
1953d65b166SJames Wright 
196f0b65372SJed Brown   const BlasiusContext           context     = (BlasiusContext)ctx;
197*512c8ec7SJames Wright   const NewtonianIdealGasContext gas         = &context->newtonian_ctx;
198ade49511SJames Wright   const bool                     is_implicit = context->implicit;
199*512c8ec7SJames Wright   const CeedScalar               Rd          = GasConstant(gas);
200*512c8ec7SJames Wright   const CeedScalar               gamma       = HeatCapacityRatio(gas);
201*512c8ec7SJames Wright   const CeedScalar               rho_0       = context->P0 / (Rd * context->T_inf);
202*512c8ec7SJames Wright   const CeedScalar               x0          = context->U_inf * rho_0 / (gas->mu * 25 / (Square(context->delta0)));
203f0b65372SJed Brown 
2043d65b166SJames Wright   CeedPragmaSIMD for (CeedInt i = 0; i < Q; i++) {
205ade49511SJames Wright     CeedScalar wdetJb, norm[3];
206ade49511SJames Wright     QdataBoundaryUnpack_3D(Q, i, q_data_sur, &wdetJb, NULL, norm);
207ade49511SJames Wright     wdetJb *= is_implicit ? -1. : 1.;
208f0b65372SJed Brown 
209f0b65372SJed Brown     // Calculate inflow values
2100d850f2eSLeila Ghaffari     const CeedScalar x[3] = {X[0][i], X[1][i], X[2][i]};
211f0b65372SJed Brown     CeedScalar       t12;
212e0d1a4dfSLeila Ghaffari     State            s = BlasiusSolution(context, x, x0, 0, rho_0, &t12);
213f0b65372SJed Brown 
214f0b65372SJed Brown     // enabling user to choose between weak T and weak rho inflow
215f0b65372SJed Brown     CeedScalar drho, dE, dP;
216*512c8ec7SJames Wright     if (context->weakT) {
217f0b65372SJed Brown       // rho should be from the current solution
218f0b65372SJed Brown       drho                   = dq[0][i];
219*512c8ec7SJames Wright       CeedScalar dE_internal = drho * gas->cv * context->T_inf;
220e0d1a4dfSLeila Ghaffari       CeedScalar dE_kinetic  = .5 * drho * Dot3(s.Y.velocity, s.Y.velocity);
221f0b65372SJed Brown       dE                     = dE_internal + dE_kinetic;
222*512c8ec7SJames Wright       dP                     = drho * Rd * context->T_inf;  // interior rho with exterior T
223f0b65372SJed Brown     } else {                                                // rho specified, E_internal from solution
224f0b65372SJed Brown       drho = 0;
225f0b65372SJed Brown       dE   = dq[4][i];
226f0b65372SJed Brown       dP   = dE * (gamma - 1.);
227f0b65372SJed Brown     }
228f0b65372SJed Brown 
229e0d1a4dfSLeila Ghaffari     const CeedScalar u_normal = Dot3(norm, s.Y.velocity);
230f0b65372SJed Brown 
231f0b65372SJed Brown     v[0][i] = -wdetJb * drho * u_normal;
2322b916ea7SJeremy L Thompson     for (int j = 0; j < 3; j++) {
233e0d1a4dfSLeila Ghaffari       v[j + 1][i] = -wdetJb * (drho * u_normal * s.Y.velocity[j] + norm[j] * dP);
2342b916ea7SJeremy L Thompson     }
235f0b65372SJed Brown     v[4][i] = -wdetJb * u_normal * (dE + dP);
236ade49511SJames Wright   }
237f0b65372SJed Brown   return 0;
238f0b65372SJed Brown }
239