Radiative torques: Analytical Model and Basic Properties

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dc.creatorLazarian, Alex
dc.creatorHoang, Thiem
dc.date2007-07-05
dc.date2007-07-24
dc.date.accessioned2026-07-07T10:56:37Z
dc.date.available2026-07-07T10:56:37Z
dc.descriptionWe attempt to get a physical insight into grain alignment processes by studying basic properties of radiative torques (RATs). For this purpose we consider a simple toy model of a helical grain that reproduces well the basic features of RATs. The model grain consists of a spheroidal body with a mirror attached at an angle to it. Being very simple, the model allows analytical description of RATs that act upon it. We show a good correspondence of RATs obtained for this model and those of irregular grains calculated by DDSCAT. Our analysis of the role of different torque components for grain alignment reveals that one of the three RAT components does not affect the alignment, but induces only for grain precession. The other two components provide a generic alignment with grain long axes perpendicular to the radiation direction, if the radiation dominates the grain precession, and perpendicular to magnetic field, otherwise. We study a self-similar scaling of RATs as a function of $λ/a_{eff}$. We show that the self-similarity is useful for studying grain alignment by a broad spectrum of radiation, i.e. interstellar radiation field.
dc.description40 pages, 50 figures
dc.identifierhttps://arxiv.org/abs/0707.0886
dc.identifierhttp://arxiv.org/abs/0707.0886
dc.identifierMon.Not.Roy.Astron.Soc.378:910,2007
dc.identifierdoi:10.1111/j.1365-2966.2007.11817.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186472
dc.subjectAstrophysics
dc.titleRadiative torques: Analytical Model and Basic Properties
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