Book contents
- Frontmatter
- Contents
- Preface
- Conference participants
- Conference photograph / poster
- 1 Physics of H2 and HD
- Astrophysical Importance of H2
- Radiative and Electronic Excitation of Lyman and Werner Transitions in H2
- The Cooling of Astrophysical Media by H2 and HD
- Highly Excited Singlet Ungerade States of H2 and their Theoretical Description
- Laboratory Studies of Long-range Excited States of H2
- A Model of Interstellar Dark Matter
- Mass of H2 Dark Matter in the Galactic Halo
- 2 Formation - Destruction
- 3 Observations and Models
- 4 Extragalactic and Cosmology
- 5 Outlook
- Author index
Laboratory Studies of Long-range Excited States of H2
from 1 - Physics of H2 and HD
Published online by Cambridge University Press: 04 August 2010
- Frontmatter
- Contents
- Preface
- Conference participants
- Conference photograph / poster
- 1 Physics of H2 and HD
- Astrophysical Importance of H2
- Radiative and Electronic Excitation of Lyman and Werner Transitions in H2
- The Cooling of Astrophysical Media by H2 and HD
- Highly Excited Singlet Ungerade States of H2 and their Theoretical Description
- Laboratory Studies of Long-range Excited States of H2
- A Model of Interstellar Dark Matter
- Mass of H2 Dark Matter in the Galactic Halo
- 2 Formation - Destruction
- 3 Observations and Models
- 4 Extragalactic and Cosmology
- 5 Outlook
- Author index
Summary
Present day laser technology has advanced such that multiple resonance excitation can be performed using several lasers of various wavelengths. Also narrowband tunable extreme ultraviolet laser radiation is readily available, to bridge the gap between the low-lying electronic ground state and the excited singlet states in molecular hydrogen. These methods have been employed to investigate a new class of excited states of H2 that are confined to large internuclear separation.
Introduction
Molecular hydrogen, the smallest neutral chemical entity, is often considered to be the simplest molecule. For a spectroscopist, however, H2 brings about a number of complications which make it a difficult object to study. First of all, from an experimental perspective, the electronic ground state is separated from the excited states by a large energy gap, which can be bridged only by photons in the domain of the extreme ultraviolet (XUV). Furthermore hydrogen is a light molecule with a very open rotational structure; the rotational lines are often so widely spaced that it is not obvious that they form a progression. Also, as a consequence of the small mass, deviations from the Born-Oppenheimer are most prominent and strongest in H2. Non-adiabatic interactions shift the energy levels over several tens of cm−1, so that the rovibronic structure becomes confused. As a result assignment of observed spectra, even with rotational quantum numbers only, is not straightforward. This point is illustrated by the Dieke atlas (Crosswhite 1972), a compilation of spectra pertaining to transitions between excited states, recorded in the visible domain with a classical spectrometer.
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- Molecular Hydrogen in Space , pp. 39 - 46Publisher: Cambridge University PressPrint publication year: 2000