
Kirchhoff’s Law of Thermal Radiation: 150 Years starts off by:
- Kirchhoff’s law is one of the simplest and most misunderstood in thermodynamics.
Let us see what we can say about Kirchhoff’s Radiation Law stating that the emissivity and absorptivity of a radiating body are equal, in the setting of the wave model with damping presented in Computational Blackbody Radiation and Mathematical Physics of Blackbody Radiation:
where the subindices indicate differentiation with respect to space
and time
, and
models a vibrating material string with
displacement
is a dissipative term modeling outgoing radiation
is a dissipative term modeling internal heating by friction
is the amplitude of the incoming forcing,
is temperature with
,
- the wave equation expresses a balance of forces,
where
and
are certain small damping coefficients defined by spectral decomposition as follows in a model case:
if the frequency 
if the frequency
,
where
represents a “smallest coordination length” depending on temperature
and
is a fixed smallest mesh size (representing some atomic dimension).
This represents a switch from outgoing radiation to internal heating as the frequency
passes the threshold
, with the threshold increasing linearly with
.
The idea is that a hotter vibrating string is capable of radiating higher frequencies as coherent outgoing radiation. The switch acts as a band filter with frequencies outside the band being stored as internal heat instead of being radiated: The radiator is then muted and heats up internally instead of delivering outgoing radiating.
A spectral analysis, assuming that all frequencies share a common temperature, shows an energy balance between incoming forcing
measured as
assuming periodicity in space and time and integrating over periods, and (rate of) outgoing radiation
measured by
,
and (rate of) internal energy measured by
,
together with the oscillator energy
with the energy balance in stationary state with
constant taking the form
with
is a constant independent of
,
,
and
. In other words,
- incoming energy =
outgoing radiation energy for 
- incoming energy =
stored internal energy for
,
which can be viewed as an expression of Kirchhoffs’ law that emissivity equals absorptivity.
The equality results from the independence of the coefficient
of the damping coefficients
and
, and frequency.
Summary: The energy of damping from outgoing radiation or internal heating is the same even if the damping terms represent different physics (emission and absorption) and have different coefficients (
and
).
PS: Note that internal heat energy accumulating under (high-frequency) forcing above cut-off eventually will be transformed into low-frequency outgoing radiation, but this transformation is not part of the above model.