An algorithm for Monte-Carlo time-dependent radiation transfer
T. Harries. (2011)cite arxiv:1105.5571Comment: 10 pages, 10 figures, accepted for publication by MNRAS.
Abstract
A new Monte-Carlo algorithm for calculating time-dependent radiative-transfer
under the assumption of LTE is presented. Unlike flux-limited diffusion the
method is polychromatic, includes scattering, and is able to treat the
optically thick and free-streaming regimes simultaneously. The algorithm is
tested on a variety of 1-d and 2-d problems, and good agreement with benchmark
solutions is found. The method is used to calculate the time-varying spectral
energy distribution from a circumstellar disc illuminated by a protostar whose
accretion luminosity is varying. It is shown that the time lag between the
optical variability and the infrared variability results from a combination of
the photon travel time and the thermal response in the disc, and that the lag
is an approximately linear function of wavelength.
Description
[1105.5571] An algorithm for Monte-Carlo time-dependent radiation transfer
%0 Generic
%1 Harries2011
%A Harries, Tim J.
%D 2011
%K RadTran montecarlo
%T An algorithm for Monte-Carlo time-dependent radiation transfer
%U http://arxiv.org/abs/1105.5571
%X A new Monte-Carlo algorithm for calculating time-dependent radiative-transfer
under the assumption of LTE is presented. Unlike flux-limited diffusion the
method is polychromatic, includes scattering, and is able to treat the
optically thick and free-streaming regimes simultaneously. The algorithm is
tested on a variety of 1-d and 2-d problems, and good agreement with benchmark
solutions is found. The method is used to calculate the time-varying spectral
energy distribution from a circumstellar disc illuminated by a protostar whose
accretion luminosity is varying. It is shown that the time lag between the
optical variability and the infrared variability results from a combination of
the photon travel time and the thermal response in the disc, and that the lag
is an approximately linear function of wavelength.
@misc{Harries2011,
abstract = { A new Monte-Carlo algorithm for calculating time-dependent radiative-transfer
under the assumption of LTE is presented. Unlike flux-limited diffusion the
method is polychromatic, includes scattering, and is able to treat the
optically thick and free-streaming regimes simultaneously. The algorithm is
tested on a variety of 1-d and 2-d problems, and good agreement with benchmark
solutions is found. The method is used to calculate the time-varying spectral
energy distribution from a circumstellar disc illuminated by a protostar whose
accretion luminosity is varying. It is shown that the time lag between the
optical variability and the infrared variability results from a combination of
the photon travel time and the thermal response in the disc, and that the lag
is an approximately linear function of wavelength.
},
added-at = {2011-05-30T19:02:34.000+0200},
author = {Harries, Tim J.},
biburl = {https://www.bibsonomy.org/bibtex/2861b7f4ab51c50fcd6f0bfc5ed7eda27/miki},
description = {[1105.5571] An algorithm for Monte-Carlo time-dependent radiation transfer},
interhash = {7f1a8e804e9c312554492d5f7dac06f6},
intrahash = {861b7f4ab51c50fcd6f0bfc5ed7eda27},
keywords = {RadTran montecarlo},
note = {cite arxiv:1105.5571Comment: 10 pages, 10 figures, accepted for publication by MNRAS},
timestamp = {2011-05-30T19:02:35.000+0200},
title = {An algorithm for Monte-Carlo time-dependent radiation transfer},
url = {http://arxiv.org/abs/1105.5571},
year = 2011
}