
TL;DR
This paper derives a relativistic variable Eddington factor in radiative flows, showing it depends on velocity and its gradient, and introduces the concept of a one-tau photo-oval affecting radiation anisotropy.
Contribution
The paper analytically derives a relativistic Eddington factor considering velocity gradients and introduces the concept of a one-tau photo-oval affecting radiation fields.
Findings
Eddington factor depends on velocity gradient and flow velocity.
The shape of the optical depth surface becomes an oval (photo-oval).
Analytic expression for Eddington factor in optically thick flows.
Abstract
We analytically derive a relativistic variable Eddington factor in the relativistic radiative flow, and found that the Eddington factor depends on the {\it velocity gradient} as well as the flow velocity. When the gaseous flow is accelerated and there is a velocity gradient, there also exists a density gradient. As a result, an unobstructed viewing range by a comoving observer, where the optical depth measured from the comoving observer is unity, is not a sphere, but becomes an oval shape elongated in the direction of the flow; we call it a {\it one-tau photo-oval}. For the comoving observer, an inner wall of the photo-oval generally emits at a non-uniform intensity, and has a relative velocity. Thus, the comoving radiation fields observed by the comoving observer becomes {\it anisotropic}, and the Eddington factor must deviate from the value for the isotropic radiation fields. % In the…
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