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The co-moving frame radiative transfer equation for spherically
symmetric flows can be written
as :
We set c=1;
is the velocity; and
is the usual Lorentz factor.
Equation
is a integro-differential equation, since the
emissivity
contains J_
, the zeroth angular moment of
I_
:

and

where
is the source function,
is the absorption
opacity, and
is the scattering opacity.
With
the assumption of time-independence
and a monotonic velocity field Eq. 1 becomes a boundary-value problem in
the spatial coordinate and an initial value problem in the frequency
or wavelength coordinate. The equation can be written in operator form
as:
where
is the lambda-operator.
Peter H. Hauschildt
4/27/1999