| /libCEED/examples/petsc/qfunctions/bps/ |
| H A D | bp4sphere.h | 27 const CeedScalar R = context[0]; in SetupDiffRhs3() local 35 x *= R / rad; in SetupDiffRhs3() 36 y *= R / rad; in SetupDiffRhs3() 37 z *= R / rad; in SetupDiffRhs3() 39 const CeedScalar theta = asin(z / R); // latitude in SetupDiffRhs3() 51 rhs[i + 0 * Q] = q_data[i + Q * 0] * 2 * sin(lambda) * cos(theta) / (R * R); in SetupDiffRhs3()
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| H A D | bp3sphere.h | 150 const CeedScalar R = context[0]; in SetupDiffRhs() local 158 x *= R / rad; in SetupDiffRhs() 159 y *= R / rad; in SetupDiffRhs() 160 z *= R / rad; in SetupDiffRhs() 162 const CeedScalar theta = asin(z / R); // latitude in SetupDiffRhs() 167 rhs[i + Q * 0] = q_data[i + Q * 0] * 2 * sin(lambda) * cos(theta) / (R * R); in SetupDiffRhs()
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| H A D | bp2sphere.h | 27 const CeedScalar R = context[0]; in SetupMassRhs3() local 32 const CeedScalar theta = asin(X[i + 2 * Q] / R); in SetupMassRhs3()
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| H A D | bp1sphere.h | 114 const CeedScalar R = context[0]; in SetupMassRhs() local 119 const CeedScalar theta = asin(X[i + 2 * Q] / R); in SetupMassRhs()
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| /libCEED/backends/sycl/ |
| H A D | ceed-sycl-common.hpp | 26 template <typename R, class... Args> 27 int CeedSetBackendFunctionCpp(Ceed ceed, const char *type, void *object, const char *fname, R (*f)(… in CeedSetBackendFunctionCpp() 28 static_assert(std::is_same_v<int, R>, "Ceed backend functions must return int"); in CeedSetBackendFunctionCpp()
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| /libCEED/examples/fluids/qfunctions/ |
| H A D | taylorgreen.h | 24 CeedScalar R = GasConstant(gas); in ICsTaylorGreen() local 27 const CeedScalar density0 = reference.pressure / (reference.temperature * R); in ICsTaylorGreen()
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| H A D | newtonian_state.h | 271 StateConservative R = {0}; in StateConservativeMult() local 273 R.density += a[i] * X[i].density; in StateConservativeMult() 274 for (int j = 0; j < 3; j++) R.momentum[j] += a[i] * X[i].momentum[j]; in StateConservativeMult() 275 R.E_total += a[i] * X[i].E_total; in StateConservativeMult() 277 return R; in StateConservativeMult() 282 StateConservative R; in StateConservativeAXPBYPCZ() local 283 R.density = a * X.density + b * Y.density + c * Z.density; in StateConservativeAXPBYPCZ() 284 …for (int i = 0; i < 3; i++) R.momentum[i] = a * X.momentum[i] + b * Y.momentum[i] + c * Z.momentum… in StateConservativeAXPBYPCZ() 285 R.E_total = a * X.E_total + b * Y.E_total + c * Z.E_total; in StateConservativeAXPBYPCZ() 286 return R; in StateConservativeAXPBYPCZ()
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| H A D | eulervortex.h | 74 const CeedScalar R = 1.; in Exact_Euler() local 137 rho = P / (R * T); in Exact_Euler() 150 rho = P / (R * T); in Exact_Euler() 164 rho = P / (R * T); in Exact_Euler() 537 const CeedScalar R = 1.; in TravelingVortex_Inflow() local 564 const CeedScalar rho_inlet = P_inlet / (R * T_inlet); in TravelingVortex_Inflow()
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| /libCEED/ |
| H A D | AUTHORS | 2 Zachary R. Atkins
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| /libCEED/doc/sphinx/source/ |
| H A D | references.bib | 53 author = {Hughes, Thomas J R and Scovazzi, Guglielmo and Tezduyar, Tayfun E}, 93 …author = {Straka, Jerry M and Wilhelmson, Robert B and Wicker, Louis J and Anderson, John R and… 196 …author = {Shur, Michael L. and Spalart, Philippe R. and Strelets, Michael K. and Travin, Andrey K… 287 author = {Bull, Jonathan R. and Jameson, Antony}, 298 author = {Van Driest, E. R.},
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| H A D | libCEEDapi.md | 21 where $\bm{x} \in \mathbb{R}^d \supset \Omega$. 31 …-component problems in $d$ dimensions, $\bm f_0 \in \mathbb{R}^n$ and $\bm f_1 \in \mathbb{R}^{nd}…
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| /libCEED/examples/petsc/src/ |
| H A D | libceedsetup.c | 55 CeedScalar R = 1; // radius of the sphere in SetupLibceedByDegree() local 170 CeedScalar rhs_setup_data[2] = {R, l}; in SetupLibceedByDegree() 253 CeedScalar R = 1; // radius of the sphere in SetupErrorOperator() local 322 CeedScalar rhs_setup_data[2] = {R, l}; in SetupErrorOperator()
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| H A D | swarmutils.c | 593 CeedScalar R = 1; // radius of the sphere in SetupProblemSwarm() local 744 CeedScalar rhs_setup_data[2] = {R, l}; in SetupProblemSwarm()
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| /libCEED/examples/ |
| H A D | notation.md | 7 We discretize the domain, $\Omega \subset \mathbb{R}^d$ (with $d=1,2,3$, typically) by letting $\Om…
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| /libCEED/doc/papers/joss/ |
| H A D | paper.bib | 155 journal={SIAM {R}eview}, 218 author = {R. Anderson and J. Andrej and A. Barker and J. Bramwell and J.-S. Camier and 251 author = {Charles R. Harris and K. Jarrod Millman and St{'{e}}fan J. 257 R{'{\i}}o and Mark Wiebe and Pearu Peterson and Pierre 325 …author={Straka, Jerry M and Wilhelmson, Robert B and Wicker, Louis J and Anderson, John R and Droe…
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| /libCEED/examples/fluids/problems/ |
| H A D | blasius.c | 20 PetscErrorCode CompressibleBlasiusResidual(SNES snes, Vec X, Vec R, void *ctx) { in CompressibleBlasiusResidual() argument 34 PetscCall(VecGetArray(R, &r)); in CompressibleBlasiusResidual() 72 PetscCall(VecRestoreArray(R, &r)); in CompressibleBlasiusResidual()
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| /libCEED/examples/solids/ |
| H A D | elasticity.c | 55 Vec R, R_loc, F, F_loc; // g: global, loc: local in main() local 204 PetscCall(VecDuplicate(U_g[fine_level], &R)); in main() 410 PetscCall(SNESSetFunction(snes, R, FormResidual_Ceed, res_ctx)); in main() 849 PetscCall(VecDestroy(&R)); in main()
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| H A D | index.md | 83 Here, we define a strain energy density functional $\Phi(\bm \epsilon) \in \mathbb R$ and obtain th…
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| /libCEED/examples/petsc/ |
| H A D | index.md | 10 …at the physical coordinates for this problem are $\bm{x}=(x,y,z)\in \mathbb{R}^3$, while the coord… 125 … a two-dimensional closed surface embedded in the three-dimensional Euclidean space $\mathbb{R}^3$.
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| /libCEED/examples/fluids/ |
| H A D | index.md | 206 In both {eq}`eq-weak-vector-ns-su` and {eq}`eq-weak-vector-ns-supg`, $\bm\tau \in \mathbb R^{5\time… 437 …overline \phi$ the filtered scalar solution field, $\bm{\Delta} \in \mathbb{R}^{3 \times 3}$ a sym… 567 …for this problem is $\rho=1$, $P=1$, $T=P/\rho= 1$ (Specific Gas Constant, $R$, is 1), and $\bm{u}… 733 tensor $\bm{C}$ (such that $\bm{R} = \bm{CC}^T$ ), bulk velocity $U_0$, 859 | $\bm{R}$ | R_ij | Yes | No | 916 \rho &= \frac{p}{R T_0} \\
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| /libCEED/examples/python/ |
| H A D | tutorial-6-shell.ipynb | 27 "We discretize the domain, $\\Omega \\subset \\mathbb{R}^d$ (with $d=1,2,3$,\n",
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