Hydrogen molecular ions: H3+, H5+ and beyond

被引：5

作者：

Tennyson, Jonathan ^{[1
]}

Miller, Steve ^{[1
]}

机构：

[1] UCL, Dept Phys & Astron, London WC1E 6BT, England

来源：

PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES | 2019年 / 377卷 / 2154期

基金：

英国工程与自然科学研究理事会;

关键词：

planetary atmospheres; interstellar medium; spectroscopy; reaction dynamics; INFRARED PREDISSOCIATION SPECTRUM; EXTREME ULTRAVIOLET OBSERVATIONS; POTENTIAL-ENERGY SURFACE; DISSOCIATIVE RECOMBINATION; UPPER-ATMOSPHERE; BROWN DWARF; H-3+; SPECTROSCOPY; EMISSION; CHEMISTRY;

D O I：

10.1098/rsta.2018.0395

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Three decades after the spectroscopic detection of H-3(+) in space, the inspiring developments in physics, chemistry and astronomy of H-n(+) (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-3(+), H-5(+) and beyond'.

引用

页数：11

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