xref: /honee/qfunctions/stabilization.h (revision edcfef1b6f4e32859128041f533d18dbf23dee67)
1 // Copyright (c) 2017-2022, Lawrence Livermore National Security, LLC and other CEED contributors.
2 // All Rights Reserved. See the top-level LICENSE and NOTICE files for details.
3 //
4 // SPDX-License-Identifier: BSD-2-Clause
5 //
6 // This file is part of CEED:  http://github.com/ceed
7 
8 /// @file
9 /// Helper functions for computing stabilization terms of a newtonian simulation
10 
11 #ifndef stabilization_h
12 #define stabilization_h
13 
14 #include <ceed.h>
15 
16 #include "newtonian_state.h"
17 
18 // *****************************************************************************
19 // Helper function for computing the variation in primitive variables, given Tau_d
20 // *****************************************************************************
21 CEED_QFUNCTION_HELPER void dYFromTau(CeedScalar Y[5], CeedScalar Tau_d[3], CeedScalar dY[5]) {
22   dY[0] = Tau_d[0] * Y[0];
23   dY[1] = Tau_d[1] * Y[1];
24   dY[2] = Tau_d[1] * Y[2];
25   dY[3] = Tau_d[1] * Y[3];
26   dY[4] = Tau_d[2] * Y[4];
27 }
28 
29 // *****************************************************************************
30 // Helper functions for computing the stabilization terms
31 // *****************************************************************************
32 CEED_QFUNCTION_HELPER void StabilizationMatrix(NewtonianIdealGasContext gas, State s, CeedScalar Tau_d[3], CeedScalar R[5],
33                                                CeedScalar stab[5][3]) {
34   CeedScalar        dY[5];
35   StateConservative dF[3];
36   // Zero stab so all future terms can safely sum into it
37   for (CeedInt i = 0; i < 5; i++) {
38     for (CeedInt j = 0; j < 3; j++) stab[i][j] = 0;
39   }
40   dYFromTau(R, Tau_d, dY);
41   State ds = StateFromY_fwd(gas, s, dY);
42   FluxInviscid_fwd(gas, s, ds, dF);
43   for (CeedInt i = 0; i < 3; i++) {
44     CeedScalar dF_i[5];
45     UnpackState_U(dF[i], dF_i);
46     for (CeedInt j = 0; j < 5; j++) stab[j][i] += dF_i[j];
47   }
48 }
49 
50 CEED_QFUNCTION_HELPER void Stabilization(NewtonianIdealGasContext gas, State s, CeedScalar Tau_d[3], State ds[3], CeedScalar U_dot[5],
51                                          const CeedScalar body_force[5], CeedScalar stab[5][3]) {
52   // -- Stabilization method: none (Galerkin), SU, or SUPG
53   CeedScalar R[5] = {0};
54   switch (gas->stabilization) {
55     case STAB_NONE:
56       break;
57     case STAB_SU:
58       FluxInviscidStrong(gas, s, ds, R);
59       break;
60     case STAB_SUPG:
61       FluxInviscidStrong(gas, s, ds, R);
62       for (CeedInt j = 0; j < 5; j++) R[j] += U_dot[j] - body_force[j];
63       break;
64   }
65   StabilizationMatrix(gas, s, Tau_d, R, stab);
66 }
67 
68 // *****************************************************************************
69 // Helper function for computing Tau elements (stabilization constant)
70 //   Model from:
71 //     PHASTA
72 //
73 //   Tau[i] = itau=0 which is diagonal-Shakib (3 values still but not spatial)
74 // *****************************************************************************
75 CEED_QFUNCTION_HELPER void Tau_diagPrim(NewtonianIdealGasContext gas, State s, const CeedScalar dXdx[3][3], const CeedScalar dt,
76                                         CeedScalar Tau_d[3]) {
77   // Context
78   const CeedScalar Ctau_t = gas->Ctau_t;
79   const CeedScalar Ctau_v = gas->Ctau_v;
80   const CeedScalar Ctau_C = gas->Ctau_C;
81   const CeedScalar Ctau_M = gas->Ctau_M;
82   const CeedScalar Ctau_E = gas->Ctau_E;
83   const CeedScalar cv     = gas->cv;
84   const CeedScalar mu     = gas->mu;
85   const CeedScalar u[3]   = {s.Y.velocity[0], s.Y.velocity[1], s.Y.velocity[2]};
86   const CeedScalar rho    = s.U.density;
87 
88   CeedScalar gijd[6];
89   CeedScalar tau;
90   CeedScalar dts;
91   CeedScalar fact;
92 
93   gijd[0] = dXdx[0][0] * dXdx[0][0] + dXdx[1][0] * dXdx[1][0] + dXdx[2][0] * dXdx[2][0];
94 
95   gijd[1] = dXdx[0][0] * dXdx[0][1] + dXdx[1][0] * dXdx[1][1] + dXdx[2][0] * dXdx[2][1];
96 
97   gijd[2] = dXdx[0][1] * dXdx[0][1] + dXdx[1][1] * dXdx[1][1] + dXdx[2][1] * dXdx[2][1];
98 
99   gijd[3] = dXdx[0][0] * dXdx[0][2] + dXdx[1][0] * dXdx[1][2] + dXdx[2][0] * dXdx[2][2];
100 
101   gijd[4] = dXdx[0][1] * dXdx[0][2] + dXdx[1][1] * dXdx[1][2] + dXdx[2][1] * dXdx[2][2];
102 
103   gijd[5] = dXdx[0][2] * dXdx[0][2] + dXdx[1][2] * dXdx[1][2] + dXdx[2][2] * dXdx[2][2];
104 
105   dts = Ctau_t / dt;
106 
107   tau = rho * rho *
108             ((4. * dts * dts) + u[0] * (u[0] * gijd[0] + 2. * (u[1] * gijd[1] + u[2] * gijd[3])) + u[1] * (u[1] * gijd[2] + 2. * u[2] * gijd[4]) +
109              u[2] * u[2] * gijd[5]) +
110         Ctau_v * mu * mu *
111             (gijd[0] * gijd[0] + gijd[2] * gijd[2] + gijd[5] * gijd[5] + +2. * (gijd[1] * gijd[1] + gijd[3] * gijd[3] + gijd[4] * gijd[4]));
112 
113   fact = sqrt(tau);
114 
115   Tau_d[0] = Ctau_C * fact / (rho * (gijd[0] + gijd[2] + gijd[5])) * 0.125;
116 
117   Tau_d[1] = Ctau_M / fact;
118   Tau_d[2] = Ctau_E / (fact * cv);
119 
120   // consider putting back the way I initially had it
121   // Ctau_E * Tau_d[1] /cv to avoid a division if the compiler is smart enough to see that cv IS a constant that it could invert once for all elements
122   // but in that case energy tau is scaled by the product of Ctau_E * Ctau_M
123   // OR we could absorb cv into Ctau_E but this puts more burden on user to know how to change constants with a change of fluid or units.  Same for
124   // Ctau_v * mu * mu IF AND ONLY IF we don't add viscosity law =f(T)
125 }
126 
127 // *****************************************************************************
128 
129 #endif  // stabilization_h
130