Tennyson Jonathan, Miller Steve
Department of Physics and Astronomy, University College London, London WC1E 6BT, UK.
Philos Trans A Math Phys Eng Sci. 2019 Sep 23;377(2154):20180395. doi: 10.1098/rsta.2018.0395. Epub 2019 Aug 5.
Three decades after the spectroscopic detection of H in space, the inspiring developments in physics, chemistry and astronomy of H (n = 3, 5, 7) systems, which led to this Royal Society Discussion Meeting, are reviewed, the present state of the art as represented by the meeting surveyed and future lines of research considered. This article is part of a discussion meeting issue 'Advances in hydrogen molecular ions: H, H and beyond'.
在太空中通过光谱法检测到氢(H)三十年之后,本文回顾了导致本次皇家学会讨论会的氢(n = 3、5、7)体系在物理、化学和天文学方面令人鼓舞的进展,审视了本次会议所代表的当前技术水平,并考虑了未来的研究方向。本文是“氢分子离子的进展:H₂⁺、H₃⁺及其他”讨论会特刊的一部分。