arXiv Analytics

Sign in

arXiv:1407.3135 [astro-ph.HE]AbstractReferencesReviewsResources

H$_{2}$O Maser Pumping: The Effect of Quasi-Resonance Energy Transfer in Collisions between H$_2$ and H$_2$O Molecules

A. V. Nesterenok, D. A. Varshalovich

Published 2014-07-11Version 1

The effect of quasi-resonance energy transfer in collisions between H$_2$ and H$_2$O molecules in H$_2$O maser sources is investigated. New data on the state-to-state rate coefficients for collisional transitions for H$_2$O and H$_2$ molecules are used in the calculations. The results of ortho-H$_2$O level population inversion calculations for the 22.2-, 380-, 439-, and 621-GHz transitions are presented. The ortho-H$_2$O level population inversion is shown to depend significantly on the population distribution of the para-H$_2$ $J = 0$ and $2$ rotational levels. The possibility of quasi-resonance energy transfer in collisions between H$_2$ molecules at highly excited rotational-vibrational levels and H$_2$O molecules is considered. The quasi-resonance energy transfer effect can play a significant role in pumping H$_2$O masers in the central regions of active galactic nuclei and in star-forming regions.

Comments: arXiv admin note: text overlap with arXiv:1309.7547
Journal: Published in Astronomy Letters, 2014, Vol. 40, No.7, pp. 425-434
Categories: astro-ph.HE, astro-ph.GA
Related articles: Most relevant | Search more
arXiv:2406.13072 [astro-ph.HE] (Published 2024-06-18)
Supermassive black hole formation via collisions in black hole clusters
arXiv:1709.04953 [astro-ph.HE] (Published 2017-09-14)
$e^+$ and $\bar{p}$ production in $pp$ collisions and the cosmic-ray $e^+/\bar{p}$ flux ratio
arXiv:2011.00004 [astro-ph.HE] (Published 2020-10-30)
A change of direction in pairwise neutrino conversion physics: The effect of collisions