This notebook is intended to demonstrate the basic features of the Python API for constructing input files and running OpenMC. In it, we will show how to create a basic reflective pin-cell model that is equivalent to modeling an infinite array of fuel pins. If you have never used OpenMC, this can serve as a good starting point to learn the Python API. We highly recommend having a copy of the Python API reference documentation open in another browser tab that you can refer to.
In [1]:
%matplotlib inline
import openmc
Materials in OpenMC are defined as a set of nuclides with specified atom/weight fractions. To begin, we will create a material by making an instance of the Material
class. In OpenMC, many objects, including materials, are identified by a "unique ID" that is simply just a positive integer. These IDs are used when exporting XML files that the solver reads in. They also appear in the output and can be used for identification. Since an integer ID is not very useful by itself, you can also give a material a name
as well.
In [2]:
uo2 = openmc.Material(1, "uo2")
print(uo2)
On the XML side, you have no choice but to supply an ID. However, in the Python API, if you don't give an ID, one will be automatically generated for you:
In [3]:
mat = openmc.Material()
print(mat)
We see that an ID of 2 was automatically assigned. Let's now move on to adding nuclides to our uo2
material. The Material
object has a method add_nuclide()
whose first argument is the name of the nuclide and second argument is the atom or weight fraction.
In [4]:
help(uo2.add_nuclide)
We see that by default it assumes we want an atom fraction.
In [5]:
# Add nuclides to uo2
uo2.add_nuclide('U235', 0.03)
uo2.add_nuclide('U238', 0.97)
uo2.add_nuclide('O16', 2.0)
Now we need to assign a total density to the material. We'll use the set_density
for this.
In [6]:
uo2.set_density('g/cm3', 10.0)
You may sometimes be given a material specification where all the nuclide densities are in units of atom/b-cm. In this case, you just want the density to be the sum of the constituents. In that case, you can simply run mat.set_density('sum')
.
With UO2 finished, let's now create materials for the clad and coolant. Note the use of add_element()
for zirconium.
In [7]:
zirconium = openmc.Material(2, "zirconium")
zirconium.add_element('Zr', 1.0)
zirconium.set_density('g/cm3', 6.6)
water = openmc.Material(3, "h2o")
water.add_nuclide('H1', 2.0)
water.add_nuclide('O16', 1.0)
water.set_density('g/cm3', 1.0)
An astute observer might now point out that this water material we just created will only use free-atom cross sections. We need to tell it to use an $S(\alpha,\beta)$ table so that the bound atom cross section is used at thermal energies. To do this, there's an add_s_alpha_beta()
method. Note the use of the GND-style name "c_H_in_H2O".
In [8]:
water.add_s_alpha_beta('c_H_in_H2O')
When we go to run the transport solver in OpenMC, it is going to look for a materials.xml
file. Thus far, we have only created objects in memory. To actually create a materials.xml
file, we need to instantiate a Materials
collection and export it to XML.
In [9]:
mats = openmc.Materials([uo2, zirconium, water])
Note that Materials
is actually a subclass of Python's built-in list
, so we can use methods like append()
, insert()
, pop()
, etc.
In [10]:
mats = openmc.Materials()
mats.append(uo2)
mats += [zirconium, water]
isinstance(mats, list)
Out[10]:
Finally, we can create the XML file with the export_to_xml()
method. In a Jupyter notebook, we can run a shell command by putting !
before it, so in this case we are going to display the materials.xml
file that we created.
In [11]:
mats.export_to_xml()
!cat materials.xml
Did you notice something really cool that happened to our Zr element? OpenMC automatically turned it into a list of nuclides when it exported it! The way this feature works is as follows:
Materials.cross_sections
has been set, indicating the path to a cross_sections.xml
file.Materials.cross_sections
isn't set, it looks for the OPENMC_CROSS_SECTIONS
environment variable.Let's see what happens if we change O16 in water to elemental O.
In [12]:
water.remove_nuclide('O16')
water.add_element('O', 1.0)
mats.export_to_xml()
!cat materials.xml
We see that now O16 and O17 were automatically added. O18 is missing because our cross sections file (which is based on ENDF/B-VII.1) doesn't have O18. If OpenMC didn't know about the cross sections file, it would have assumed that all isotopes exist.
cross_sections.xml
fileThe cross_sections.xml
tells OpenMC where it can find nuclide cross sections and $S(\alpha,\beta)$ tables. It serves the same purpose as MCNP's xsdir
file and Serpent's xsdata
file. As we mentioned, this can be set either by the OPENMC_CROSS_SECTIONS
environment variable or the Materials.cross_sections
attribute.
Let's have a look at what's inside this file:
In [13]:
!cat $OPENMC_CROSS_SECTIONS | head -n 10
print(' ...')
!cat $OPENMC_CROSS_SECTIONS | tail -n 10
In [14]:
uo2_three = openmc.Material()
uo2_three.add_element('U', 1.0, enrichment=3.0)
uo2_three.add_element('O', 2.0)
uo2_three.set_density('g/cc', 10.0)
At this point, we have three materials defined, exported to XML, and ready to be used in our model. To finish our model, we need to define the geometric arrangement of materials. OpenMC represents physical volumes using constructive solid geometry (CSG), also known as combinatorial geometry. The object that allows us to assign a material to a region of space is called a Cell
(same concept in MCNP, for those familiar). In order to define a region that we can assign to a cell, we must first define surfaces which bound the region. A surface is a locus of zeros of a function of Cartesian coordinates $x$, $y$, and $z$, e.g.
Between those three classes of surfaces (planes, cylinders, spheres), one can construct a wide variety of models. It is also possible to define cones and general second-order surfaces (tori are not currently supported).
Note that defining a surface is not sufficient to specify a volume -- in order to define an actual volume, one must reference the half-space of a surface. A surface half-space is the region whose points satisfy a positive or negative inequality of the surface equation. For example, for a sphere of radius one centered at the origin, the surface equation is $f(x,y,z) = x^2 + y^2 + z^2 - 1 = 0$. Thus, we say that the negative half-space of the sphere, is defined as the collection of points satisfying $f(x,y,z) < 0$, which one can reason is the inside of the sphere. Conversely, the positive half-space of the sphere would correspond to all points outside of the sphere.
Let's go ahead and create a sphere and confirm that what we've told you is true.
In [15]:
sph = openmc.Sphere(R=1.0)
Note that by default the sphere is centered at the origin so we didn't have to supply x0
, y0
, or z0
arguments. Strictly speaking, we could have omitted R
as well since it defaults to one. To get the negative or positive half-space, we simply need to apply the -
or +
unary operators, respectively.
(NOTE: Those unary operators are defined by special methods: __pos__
and __neg__
in this case).
In [16]:
inside_sphere = -sph
outside_sphere = +sph
Now let's see if inside_sphere
actually contains points inside the sphere:
In [17]:
print((0,0,0) in inside_sphere, (0,0,2) in inside_sphere)
print((0,0,0) in outside_sphere, (0,0,2) in outside_sphere)
Everything works as expected! Now that we understand how to create half-spaces, we can create more complex volumes by combining half-spaces using Boolean operators: &
(intersection), |
(union), and ~
(complement). For example, let's say we want to define a region that is the top part of the sphere (all points inside the sphere that have $z > 0$.
In [18]:
z_plane = openmc.ZPlane(z0=0)
northern_hemisphere = -sph & +z_plane
For many regions, OpenMC can automatically determine a bounding box. To get the bounding box, we use the bounding_box
property of a region, which returns a tuple of the lower-left and upper-right Cartesian coordinates for the bounding box:
In [19]:
northern_hemisphere.bounding_box
Out[19]:
Now that we see how to create volumes, we can use them to create a cell.
In [20]:
cell = openmc.Cell()
cell.region = northern_hemisphere
# or...
cell = openmc.Cell(region=northern_hemisphere)
By default, the cell is not filled by any material (void). In order to assign a material, we set the fill
property of a Cell
.
In [21]:
cell.fill = water
A collection of cells is known as a universe (again, this will be familiar to MCNP/Serpent users) and can be used as a repeatable unit when creating a model. Although we don't need it yet, the benefit of creating a universe is that we can visualize our geometry while we're creating it.
In [22]:
universe = openmc.Universe()
universe.add_cell(cell)
# this also works
universe = openmc.Universe(cells=[cell])
The Universe
object has a plot
method that will display our the universe as current constructed:
In [23]:
universe.plot(width=(2.0, 2.0))
By default, the plot will appear in the $x$-$y$ plane. We can change that with the basis
argument.
In [24]:
universe.plot(width=(2.0, 2.0), basis='xz')
If we have particular fondness for, say, fuchsia, we can tell the plot()
method to make our cell that color.
In [25]:
universe.plot(width=(2.0, 2.0), basis='xz',
colors={cell: 'fuchsia'})
We now have enough knowledge to create our pin-cell. We need three surfaces to define the fuel and clad:
These three surfaces will all be instances of openmc.ZCylinder
, each with a different radius according to the specification.
In [26]:
fuel_or = openmc.ZCylinder(R=0.39)
clad_ir = openmc.ZCylinder(R=0.40)
clad_or = openmc.ZCylinder(R=0.46)
With the surfaces created, we can now take advantage of the built-in operators on surfaces to create regions for the fuel, the gap, and the clad:
In [27]:
fuel_region = -fuel_or
gap_region = +fuel_or & -clad_ir
clad_region = +clad_ir & -clad_or
Now we can create corresponding cells that assign materials to these regions. As with materials, cells have unique IDs that are assigned either manually or automatically. Note that the gap cell doesn't have any material assigned (it is void by default).
In [28]:
fuel = openmc.Cell(1, 'fuel')
fuel.fill = uo2
fuel.region = fuel_region
gap = openmc.Cell(2, 'air gap')
gap.region = gap_region
clad = openmc.Cell(3, 'clad')
clad.fill = zirconium
clad.region = clad_region
Finally, we need to handle the coolant outside of our fuel pin. To do this, we create x- and y-planes that bound the geometry.
In [29]:
pitch = 1.26
left = openmc.XPlane(x0=-pitch/2, boundary_type='reflective')
right = openmc.XPlane(x0=pitch/2, boundary_type='reflective')
bottom = openmc.YPlane(y0=-pitch/2, boundary_type='reflective')
top = openmc.YPlane(y0=pitch/2, boundary_type='reflective')
The water region is going to be everything outside of the clad outer radius and within the box formed as the intersection of four half-spaces.
In [30]:
water_region = +left & -right & +bottom & -top & +clad_or
moderator = openmc.Cell(4, 'moderator')
moderator.fill = water
moderator.region = water_region
OpenMC also includes a factory function that generates a rectangular prism that could have made our lives easier.
In [31]:
box = openmc.get_rectangular_prism(width=pitch, height=pitch,
boundary_type='reflective')
type(box)
Out[31]:
Pay attention here -- the object that was returned is NOT a surface. It is actually the intersection of four surface half-spaces, just like we created manually before. Thus, we don't need to apply the unary operator (-box
). Instead, we can directly combine it with +clad_or
.
In [32]:
water_region = box & +clad_or
The final step is to assign the cells we created to a universe and tell OpenMC that this universe is the "root" universe in our geometry. The Geometry
is the final object that is actually exported to XML.
In [33]:
root = openmc.Universe(cells=(fuel, gap, clad, moderator))
geom = openmc.Geometry()
geom.root_universe = root
# or...
geom = openmc.Geometry(root)
geom.export_to_xml()
!cat geometry.xml
In [34]:
point = openmc.stats.Point((0, 0, 0))
src = openmc.Source(space=point)
Now let's create a Settings
object and give it the source we created along with specifying how many batches and particles we want to run.
In [35]:
settings = openmc.Settings()
settings.source = src
settings.batches = 100
settings.inactive = 10
settings.particles = 1000
In [36]:
settings.export_to_xml()
!cat settings.xml
We actually have all the required files needed to run a simulation. Before we do that though, let's give a quick example of how to create tallies. We will show how one would tally the total, fission, absorption, and (n,$\gamma$) reaction rates for $^{235}$U in the cell containing fuel. Recall that filters allow us to specify where in phase-space we want events to be tallied and scores tell us what we want to tally:
$$X = \underbrace{\int d\mathbf{r} \int d\mathbf{\Omega} \int dE}_{\text{filters}} \; \underbrace{f(\mathbf{r},\mathbf{\Omega},E)}_{\text{scores}} \psi (\mathbf{r},\mathbf{\Omega},E)$$In this case, the where is "the fuel cell". So, we will create a cell filter specifying the fuel cell.
In [37]:
cell_filter = openmc.CellFilter(fuel)
t = openmc.Tally(1)
t.filters = [cell_filter]
The what is the total, fission, absorption, and (n,$\gamma$) reaction rates in $^{235}$U. By default, if we only specify what reactions, it will gives us tallies over all nuclides. We can use the nuclides
attribute to name specific nuclides we're interested in.
In [38]:
t.nuclides = ['U235']
t.scores = ['total', 'fission', 'absorption', '(n,gamma)']
Similar to the other files, we need to create a Tallies
collection and export it to XML.
In [39]:
tallies = openmc.Tallies([t])
tallies.export_to_xml()
!cat tallies.xml
In [40]:
openmc.run()
Out[40]:
Great! OpenMC already told us our k-effective. It also spit out a file called tallies.out
that shows our tallies. This is a very basic method to look at tally data; for more sophisticated methods, see other example notebooks.
In [41]:
!cat tallies.out
We saw before that we could call the Universe.plot()
method to show a universe while we were creating our geometry. There is also a built-in plotter in the Fortran codebase that is much faster than the Python plotter and has more options. The interface looks somewhat similar to the Universe.plot()
method. Instead though, we create Plot
instances, assign them to a Plots
collection, export it to XML, and then run OpenMC in geometry plotting mode. As an example, let's specify that we want the plot to be colored by material (rather than by cell) and we assign yellow to fuel and blue to water.
In [42]:
p = openmc.Plot()
p.filename = 'pinplot'
p.width = (pitch, pitch)
p.pixels = (200, 200)
p.color_by = 'material'
p.colors = {uo2: 'yellow', water: 'blue'}
With our plot created, we need to add it to a Plots
collection which can be exported to XML.
In [43]:
plots = openmc.Plots([p])
plots.export_to_xml()
!cat plots.xml
Now we can run OpenMC in plotting mode by calling the plot_geometry()
function. Under the hood this is calling openmc --plot
.
In [44]:
openmc.plot_geometry()
Out[44]:
OpenMC writes out a peculiar image with a .ppm
extension. If you have ImageMagick installed, this can be converted into a more normal .png
file.
In [45]:
!convert pinplot.ppm pinplot.png
We can use functionality from IPython to display the image inline in our notebook:
In [46]:
from IPython.display import Image
Image("pinplot.png")
Out[46]:
That was a little bit cumbersome. Thankfully, OpenMC provides us with a function that does all that "boilerplate" work.
In [47]:
openmc.plot_inline(p)