# Thermal radiation, heat transfer, and non-equilibrium Casimir forces between silicon dioxide spheres

In this example, we use scuff-neq to compute **(1)** the
power radiated by a single SiO2 sphere, and **(2)** the heat
transfer and non-equilibrium Casimir force between two SiO2
spheres. We compare the results of scuff-neq to
the predictions of the
T-matrix formalism of Krueger et al.

The files for this example may be found in the
`share/scuff-em/examples/SiO2Spheres`

subdirectory
of your scuff-em installation.

## gmsh geometry file and surface mesh for a single sphere

The gmsh geometry file `Sphere.geo`

describes a sphere of radius 1 micron; it may
be meshed to generate coarse and fine surface meshes as follows:

```
% gmsh -2 -clscale 1 Sphere.geo
% RenameMesh Sphere.msh
% gmsh -2 -clscale 0.5 Sphere.geo
% RenameMesh Sphere.msh
```

(Here `RenameMesh`

is a simple `bash`

script
that uses scuff-analyze to count the number of interior
edges in a surface mesh and rename the mesh file accordingly.)
This produces the files `Sphere_501.msh`

and `Sphere_1479.msh,`

which you can visualize by opening in gmsh::

```
% gmsh Sphere_501.msh
```

```
% gmsh Sphere_1479.msh
```

## scuff-em geometry files

The scuff-em geometry file
`SiO2Sphere_501.scuffgeo`

describes a single SiO2 sphere.

The scuff-em geometry files
`SiO2Spheres_501.scuffgeo`

`SiO2Spheres_1479.scuffgeo`

each describe the same configuration: two SiO2 spheres
separated by a center--center distance of 10 microns.
You can visualize this configuration by typing e.g.

```
% scuff-analyze --geometry SiO2Spheres_1479.scuffgeo --WriteGMSHFiles
% gmsh SiO2Spheres_1479.pp
```

## Spectral density of radiated power

As described in the scuff-neq documentation, scuff-neq computes the total power radiated by finite-temperature objects as an integral over angular frequencies in which the integrand involves a temperature-dependent Bose-Einstein factor and a temperature-independent dimensionless flux To calculate this radiated-power flux at a given set of frequencies, we say

```
% scuff-neq --geometry SiO2Sphere_501.scuffgeo --OmegaFile --PRad
```

where `OmegaFile`

is a list of
angular frequencies. (Here `--PRad`

says that we
are interested in the radiated power).
This produces the file
`SiO2Sphere_501.SiFlux`

, which looks something
like this:

```
# scuff-neq run on superhr2 (07/11/15::00:31:36)
# data file columns:
# 1 transform tag
# 2 omega
# 3 (sourceObject,destObject)
# 4 PRad flux spectral density
DEFAULT 1.000000e-01 11 4.18911788e-06
DEFAULT 1.300000e-01 11 1.38869207e-05
DEFAULT 1.600000e-01 11 3.93335327e-05
DEFAULT 1.900000e-01 11 1.05263974e-04
```

As the file header says, the second column here
is the angular frequency
in units of rad/sec
and the fourth column is the dimensionless power
flux. (The first column lists the
geometrical transformation; since
we didn't specify the `--transfile`

option to
scuff-neq, we have just a single geometric
configuration, labeled `DEFAULT`

. The third
column identifies the source and destination objects;
since this geometry only has a single object,
the source and destination object are both
always object 1 and this column always reads
`11`

.)

Here's a plot of the data:

In this plot, the solid line is the prediction of
the Krueger formalism, as computed
by a julia code called `KruegerFormulas.jl`

.

The plot is produced by gnuplot using this script.

## Spectral density of power transfer and non-equilibrium force

Here's a bash script that runs scuff-neq
for both the coarsely-meshed and finely-meshed two-sphere
geometry to compute the fluxes of power transfer
and nonequilibrium force between the spheres.
Running the script produces files `SiO2Spheres_501.SIFlux`

and `SiO2Spheres_1479.SIFlux.`

Here are plots (produced
by the same gnuplot script referenced above)
of the heat-transfer flux from sphere 1 to sphere 2,
and the force fluxes from sphere 1 to sphere 2 and
from sphere 2 to sphere 2, compared to the Krueger
T-matrix results (again computed using the julia
code referenced above).