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Prog. Theor. Phys. Vol. 125 No. 4 (2011) pp. 837-850
Analytical Solutions of Relativistic Plane-Parallel Flows
Jun Fukue
Astronomical Institute, Osaka Kyoiku University, Kashiwara 582-8582, Japan
(Received January 16, 2011)
Abstract:
Relativistic radiative transfer in a relativistic plane-parallel flow
is examined in the fully special relativistic treatment.
Under the assumption of a constant flow speed,
we obtain simple analytical solutions
of the relativistic radiative transfer equation
for relativistic plane-parallel flows
in the cases of linear-flow and two-stream approximations.
In both cases, the solutions exhibit exponential behavior
on the optical depth. In addition,
the optical depth τ in the exponential term
is replaced by the apparent optical depth Γτ,
where Γ is a function of the flow speed v (= βc);
for example, in the case of the linear-flow approximation,
Γ= γβ, γ being the Lorentz factor.
This modification of the apparent/effective optical depth
is an essential property of the relativistic radiative transfer.
Furthermore, in the nonrelativistic regime, the radiative intensity
in the comoving frame increases as the optical depth increases,
whereas it approaches a constant value with the optical depth
in the relativistic regime because of the exponential term.
The radiation energy density in the comoving frame
also approaches a constant value,
while the radiative flux becomes zero as the optical depth increases.
Such behavior of the radiative quantities in the comoving frame,
which originates from the exponential term,
is also an essential property of the relativistic radiative transfer.
Subject Index :
420, 425, 426, 480
URL :
http://ptp.ipap.jp/link?PTP/125/837/
DOI : 10.1143/PTP.125.837
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Citing Article(s) :
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Progress of Theoretical Physics Vol. 126 No. 1 (2011) pp. 135-155
:
-
Relativistic Milne-Eddington-Type Solutions with a Variable Eddington Factor for Relativistic Plane-Parallel Flows
-
Jun Fukue