# Spatialsolver Support – `pyne.spatialsolver`

¶

Spatialsolver is a pyne module that contains seven neutron transport equation solvers. Each solver is its own unique nodal method. The solvers included in this module are listed below. The theory and methodology behind each can be found in the theory documentation.

AHOTN-LN: Arbitrarily higher order transport method of the nodal type linear-nodal methodAHOTN-LL: Arbitrarily higher order transport method of the nodal type linear-linear methodAHOTN-NEFD: Arbitrarily higher order transport method of the nodal type that makes use of the unknown nodal flux moments (NEFD algorithm).DGFEM-LD: The Discontinuous Galerkin Finite Element Method (DGFEM) with a linear discontinuous (LD) approximation for angular flux.DGFEM-DENSE: The Discontinuous Galerkin Finite Element Method (DGFEM) that use Lagrange polynomials to create a function space in each dimension.DGFEM-LAGRANGE: The Discontinuous Galerkin Finite Element Method (DGFEM) uses Lagrange polynomials to create a function space in each dimension.SCTSTEP: SCT Step algorithm uses a step approximation in all cells that are intersected by lines and planes of non-smoothness.

## Spatialsolver API¶

As these are complicated solvers, they require a large amount of input data supplied by the user. This information needs to be entered as a Python dictionary. Of the many key-pair values listed below, most are required, but some are optional. The optional entries will be overridden by default values if not present/specified.

## Input Dictionary Entries¶

Input Dictionary Entry: Solver type (AHOTN, DGFEM or SCTSTEP)key: "solver" type: String ex: "AHOTN" default: no default Note: The three supported "solver"s are the following: 1. "AHOTN" 2. "DGFEM" 3. "SCTSTEP"

Input Dictionary Entry: Spatial expansion orderkey: "solver_type" type: String ex: "LN" default: No default Note: This entry is dependent on the "solver" entry. For AHOTN solver, there exist the "LN", "LL", and "NEFD" solver types For the DGFEM solvers, there exist the "LD", "DENSE", and "LAGRANGE" solver types For the SCTSTEP solver, the "solver_type" key is not used.

Input Dictionary Entry: Spatial expansion order (lambda; ahot spatial order, 0, 1, or 2)key: "spatial_order" type: Integer ex: 0 default: 1 The Spatial expansion order is the expansion order of the spatial moment.

Input Dictionary Entry: Angular quadrature orderkey: "quadrature_order" type: Integer ex: 4 default: 4 The angular quadrature order is the number of angles to be used per octant. For N sets of angles, there will be (N * (N + 2) / 8) ordinates per octant. The quadrature order may only be an even number!

Input Dictionary Entry: Quadrature type:key: "quadrature_type" type: Integer ex: 1 default: 1 The quadrature type is the type of quadrature scheme the code uses. The possibilities are: 1 - TWOTRAN 2 - EQN 3 - Read-in

Input Dictionary Entry: Number of spatial nodes in x, y, and z directions (nx/ny/nz)key: "nodes_xyz" type: Integer array ex: [4, 4, 4] default: No default

Input Dictionary Entry: Number of energy groups (ng)key: "num_groups" type: Integer ex: 1 default: No default

Input Dictionary Entry: Number of materials (nm)key: "num_materials" type: Integer ex: 1 default: No default

Input Dictionary Entry: x-size of cells (dx)key: "x_cells_widths" type: double array ex: [0.25, 0.25, 0.25, 0.25] default: No default

Input Dictionary Entry: y-size of cells (dy)key: "y_cells_widths" type: double array ex: [0.25, 0.25, 0.25, 0.25] default: No default

Input Dictionary Entry: z-size of cells (dz)key: "z_cells_widths" type: double array ex: [0.25, 0.25, 0.25, 0.25] default: No default

Input Dictionary Entry: x start and end boundary conditionskey: "x_boundry_conditions" type: Integer array ex: [2, 2] default: No default 'x_boundary_conditions' are the x boundary conditions for each face of the cubic mesh. The entries are: x[0] = x starting bc; the left x[1] = x ending bc; the right The following are supported boundary conditions: 0 - vacuum 1 - reflective 2 - fixed inflow

Input Dictionary Entry: y start and end boundary conditionskey: "y_boundry_conditions" type: Integer array ex: [2, 2] default: No default 'y_boundary_conditions' are the y boundary conditions for each face of the cubic mesh. The entries are: y[0] = y starting bc; the front y[1] = y ending bc; the back The following are supported boundary conditions: 0 - vacuum 1 - reflective 2 - fixed inflow

Input Dictionary Entry: z start and end boundary conditionskey: "z_boundry_conditions" type: Integer array ex: [2, 2] default: No default 'z_boundary_conditions' are the z boundary conditions for each face of the cubic mesh. The entries are: z[0] = z starting bc; the bottom z[1] = z ending bc; the top The following are supported boundary conditions: 0 - vacuum 1 - reflective 2 - fixed inflow

Input Dictionary Entry: Material infokey: "material_id" type: Integer 3 dimensional array ex: [ [ [1 1 1 1] [1 1 1 1] [1 1 1 1] [1 1 1 1] ] [ [1 1 1 1] [1 1 1 1] [1 1 1 1] [1 1 1 1] ] [ [1 1 1 1] [1 1 1 1] [1 1 1 1] [1 1 1 1] ] ] default: No default note: Dimensions must match cells such that there is one material number in each spatial cell. The cells are ordered as x, y, z.

Input Dictionary Entry: “quadrature_file” [optional; only needed for quadrature type 2]key: "quad_file" type: String ex: 'quad_file' default: No default note: See input file formatting notes in the Quadrature File Formatting section.

Input Dictionary Entry: cross section info file namekey: "xs_file" type: String default: 'xs_file' note: See input file formatting notes in the Cross Section File Formatting section.

Input Dictionary Entry: source file namekey: "source_input_file" type: String default: 'src.dat' note: See input file formatting notes in the Source File Formatting section.

Input Dictionary Entry: boundary condition file name [optional]key: "bc_input_file" type: String default: No default note: See input file formatting notes in the Boundry Condition File Formatting section.

Input Dictionary Entry: output file name [optional]key: "flux_output_file" type: String default: 'flux.out' note: See input file formatting notes in the Flux Output (5.) File Formatting section.

Input Dictionary Entry: Convergence Criterionkey: "convergence_criterion" type: float ex: 1.e-5 default: 1.e-5 The solution is considered converged and the calculation completes when the flux in each cell at the current iteration is within "convergence_criterion" of the previous iterate. This is generally the relative difference, but in cases of very small flux values the absolute difference is used instead (see the Convergence Tolerance entry below).

Input Dictionary Entry: Tolerancekey: "converge_tolerance" type: float ex: 1.e-10 default: 1.e-10 Converge tolerance is the tolerance that determines how the difference between flux iterates (df) that is used to determine convergence will be calculated. df is calculated as follows: f = current flux value ct = convergence tolerance (value for this key, "converge_tolerance") f1 = flux value from the previous iteration If f1 > ct: df = absolute(f - f1) / f1 Else df = absolute(f - f1) The idea is to use the absolute difference instead of the relative difference between iterates when the flux is very small to help avoid rounding error.

Input Dictionary Entry: Maximum Iterationskey: "max_iterations" type: int ex: 10000 default: 10000 note: If this number of iterations is reached before the convergence criterion is satisfied, the calculation will terminate and report the current flux estimate.

Input Dictionary Entry: Moments Convergedkey: "moments_converged" type: int ex: 0 default: 0 Moments converged is the number of moments that should be converged upon for each quadrature in the solution space. Value for moments converged must be in range [0, spatial_order_in].

## Output Dictionary Entries¶

When run, the solvers return a dictionary of useful solution data. It contains the following key-pair entries:

**Output Dictionary Entry: Flux output array**

```
key: "flux"
type: Double Array of 3 dimensions
format: Flux output array is in following format:
Each cell in the array has a scalar flux, the integral of the angular
flux over all angles in that cell. The first index refers to the
plane on the z axis, beginning at 0 with the lowest plane, and moving
upwards to the highest plane on the mesh. The second index is the
row on the z plane, and the third index is the cell in the row.
format examples: If you had a mesh with 4 by 4 by 4 cells extending
in the x, y and z directions, then to get the following flux values,
you would use the following indices:
(1.) Scalar flux across top of cell 1,1,1: flux_array[1][1][1]
Geometric location of this cell:
Plane: Bottom of cube
Row: First y row (j) of cells
Cell: First cell in x direction
(2.) Scalar flux across top of cell 1,1,2: flux_array[1][1][2]
Geometric location of this cell:
Plane: Bottom of cube
Row: First y row (j) of cells
Cell: Second cell in x direction
(3.) Scalar flux across top of cell 1,2,1: flux_array[1][2][1]
Geometric location of this cell:
Plane: Bottom of cube
Row: Second y row (j) of cells
Cell: First cell in x direction
(4.) Scalar flux across top of cell 2,1,1: flux_array[2][1][1]
Geometric location of this cell:
Plane: Top of one cell up from bottom of cube
Row: First y row (j) of cells
Cell: First cell in x direction
```

**Output Dictionary Entry: Solver success code**

```
key: "success"
type: Integer
format: 1 means yes, the solve succeeded. 0 means it failed.
```

**Output Dictionary Entry: Raw system time of solver start**

```
time_start provides you with the system time when the solver began running.
key: "time_start"
type: double
format: system time
```

**Output Dictionary Entry: Total run time**

```
total_time is the total time the solver took to solve.
key: "total_time"
type: double
format: system time
```

**Output Dictionary Entry: Total print time**

```
print_time is the total time the solver took to print results.
key: "print_time"
type: double
format: system time
```

**Output Dictionary Entry: Error Message**

```
If the solver fails, error_msg is a string describing why the solver failed.
key: "error_msg"
type: String
```

**Output Dictionary Entries**

```
The output dictionary also contains all of the relevant input values found in the input dictionary. If one
of the optional input entries was not present, the default key-pair value will be present in this new output
dictionary.
```

### ::¶

### Source File Formatting¶

- The spatial solver dictionary requires multiple input binary source files. The required files are the following:
- XS file
- Source input file
- BC input file
- Quad file (optional)

Here is a brief description of how each should be (or is) formatted.

- (1.) XS file:
The xs file contains information about the cross sections for materials used. Each material should be assigned an ID, and the cross section data should be in the following format. It should be saved as either an extensionless or .txt file.

! Cross section file

! Material # 1

! Group #1

1.1 ! Total XS

0.2 ! Scattering matrix

! Material 2

…

! End Cross section file

- (2.) Source file:
The source file is a file containing source information for each cell. The formatting is dependant on the solver you select.

For the AHOTN and DGFEM solvers, the source file should be formatted as following. There should be ng * nx * ny * nz * lambda * lambda * lambda source entries present. We will refer to the index of each source value as (ng, nx, ny, nz, lambda_x, lambda_y, lambda_z). The source entries should be in the following order:

(1,1,1,1,1,1,1)

(1,1,1,1,1,1,2)

(1,1,1,1,1,1,.)

(1,1,1,1,1,2,1)

(1,1,1,1,1,2,2)

(1,1,1,1,1,2,.)

(1,1,1,1,1,.,.)

(1,1,1,1,2,1,1)

(1,1,1,1,2,1,2)

(1,1,1,1,2,1,.)

(1,1,1,1,2,2,1)

(1,1,1,1,2,2,2)

(1,1,1,1,2,2,.)

(1,1,1,1,2,.,.)

(1,1,1,1,.,.,.)

(1,1,1,2,1,1,1)

(1,1,1,2,1,1,2)

(1,1,1,2,1,1,.)

(1,1,1,2,1,2,1)

(1,1,1,2,1,2,2)

(1,1,1,2,1,2,.)

(1,1,1,2,1,.,.)

(1,1,1,2,2,1,1)

(1,1,1,2,2,1,2)

(1,1,1,2,2,1,.)

(1,1,1,2,2,2,1)

(1,1,1,2,2,2,2)

(1,1,1,2,2,2,.)

(1,1,1,2,2,.,.)

(1,1,1,.,.,.,.)

…

(1,1,.,.,.,.,.)

…

(1,.,.,.,.,.,.)

…

(.,.,.,.,.,.,.)

- When being read in, they will be iterated over by the following loop:

- DO g=1,ng

- DO ix=1,nx

- DO iy=1,ny

- DO iz=1,nz

- DO jx=0,lambda

- DO jy=0,lambda

- DO jz=0,lambda
- READ(12) s(jx,jy,jz,ix,iy,iz,g)
For the SCT STEP solver, the source file should be formatted as following. There should be ng * nx * ny * nz source entries present. We will refer to the index of each source value as (ng, nx, ny, nz). The source entries should be in the following order:

(1,1,1,1)

(1,1,1,2)

(1,1,1,.)

(1,1,2,1)

(1,1,2,2)

(1,1,2,.)

(1,1,.,.)

(1,2,1,1)

(1,2,1,2)

(1,2,1,.)

(1,2,2,1)

(1,2,2,2)

(1,2,2,.)

(1,2,.,.)

(1,.,.,.)

(2,1,1,1)

(2,1,1,2)

(2,1,1,.)

(2,1,2,1)

(2,1,2,2)

(2,1,2,.)

(2,1,.,.)

(2,2,1,1)

(2,2,1,2)

(2,2,1,.)

(2,2,2,1)

(2,2,2,2)

(2,2,2,.)

(2,2,.,.)

(.,.,.,.)

- When being read in, they will be iterated over by the following loop:

- DO g=1,ng

- DO ix=1,nx

- DO iy=1,ny

- DO iz=1,nz
- READ(12) s(ix,iy,iz,g,1,1,1)
- (3.) Boundary Condition file (only needed if one of the boundary conditions specified above is 2):
- The boundary condition file contains information about the incoming scalar flux on each face of each cell.
- (4.) Quadrature file (optional):
- If the quadrature type you selected was 2, a quadrature file is required for running the solver. If the quadrature type is not 2, no quadrature file is necessary.
- (5.) Flux output file (output & optional):
If a output file name was specified, the final flux will be printed to that file in the following format. Note that all flux values will be printed as a fortran REAL, and the termination key will be 0.0d0 (to indicate the end of the flux info)

AHOTN Solvers: Unformatted file, with all mesh scalar flux values in the following order:

NOTE ORDERING: flux(ng,nx,ny,nz,jx,jy,jz)

(0,0,0,0,0,0,0)

(0,0,0,0,0,0,1)

(0,0,0,0,0,1,0)

(0,0,0,0,0,1,1)

…

(0,0,0,0,0,.,.)

…

(0,0,0,0,.,.,.)

…

(0,0,0,nz,.,.,.)

…

(0,0,0,.,.,.,.)

…

(0,0,ny,.,.,.,.)

…

(0,0,.,.,.,.,.)

…

(0,nz,.,.,.,.,.)

…

(0,.,.,.,.,.,.)

…

(ng,.,.,.,.,.,.)

…

- DGFEM Solvers: Unformatted file, with all mesh scalar flux values in the following order:
NOTE ORDERING: flux(ng,nx,ny,nz,spatial_order,spatial_order,spatial_order)

(0,0,0,0,0,0,0)

(0,0,0,0,0,0,1)

…

(0,0,0,0,0,0,spatial_order)

(0,0,0,0,0,1,0)

(0,0,0,0,0,1,1)

…

(0,0,0,0,0,1,spatial_order)

…

(0,0,0,0,0,spatial_order,.)

…

(0,0,0,0,spatial_order,.,.)

…

(0,0,0,0,.,.,.)

…

(0,0,0,nz,.,.,.)

…

(0,0,0,.,.,.,.)

…

(0,0,ny,.,.,.,.)

…

(0,0,.,.,.,.,.)

…

(0,nz,.,.,.,.,.)

…

(0,.,.,.,.,.,.)

…

(ng,.,.,.,.,.,.)

…

SCTSTEP Solvers: SCTSTEP Currently not supported. Nothing will be printed to file (although file may still be created).

All functionality may be found in the `spatialsolver`

package:

```
from pyne import spatialsolver
```