Comment on Temperature Inversion in Long-Range Interacting Systemsстатья
Статья опубликована в высокорейтинговом журнале
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Дата последнего поиска статьи во внешних источниках: 28 октября 2016 г.
Аннотация:In the recent paper by Teles et al. [Phys. Rev. E 92, 020101 (2015)], it was suggested that the inversed temperature profiles in various astrophysical objects — ranging from the solar corona to the interstellar molecular clouds — can be explained by the specific features of relaxation in the long-range interacting systems. Here, we show that this mechanism can really work in the self-gravitating interstellar gaseous clouds; but it is irrelevant in the solar (and stellar) coronas where stratification of density is produced by the external gravitational field.