Abstract
The spin temperature of neutral hydrogen, which determines the optical depth and brightness of the 21-cm line, is determined by the competition between radiative and collisional processes. Here, we examine the role of proton-hydrogen collisions in setting the spin temperature. We use recent fully quantum-mechanical calculations of the relevant cross-sections, which allow us to present accurate results over the entire physically relevant temperature range 1-104 K. For kinetic temperatures TK ≳ 100 K, the proton-hydrogen rate coefficient exceeds that for hydrogen-hydrogen collisions by about a factor of 2. However, at low temperatures (TK ≲ 5 K) H-H+ collisions become several thousand times more efficient than H-H and even more important than H-e- collisions. © 2007 RAS.
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Furlanetto, S. R., & Furlanetto, M. R. (2007). Spin exchange rates in proton-hydrogen collisions. Monthly Notices of the Royal Astronomical Society, 379(1), 130–134. https://doi.org/10.1111/j.1365-2966.2007.11921.x
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