A Molecular Candle Where Few Molecules Shine: HeHHe+
Autor: | Ben Khalifa, M., Quintas-Sánchez, E., Dawes, R., Hammami, K., Fortenberry, Ryan, Wiesenfeld, Laurent |
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Přispěvatelé: | Laboratoire Aimé Cotton (LAC), CNRS-Université de Paris-Sud |
Rok vydání: | 2020 |
Předmět: |
Extraterrestrial Environment
Infrared media_common.quotation_subject Pharmaceutical Science Infrared spectroscopy Astrophysics::Cosmology and Extragalactic Astrophysics Helium Vibration 01 natural sciences Molecular physics Quantum chemistry Article Analytical Chemistry quantum chemistry lcsh:QD241-441 Isotopes lcsh:Organic chemistry Spectroscopy Fourier Transform Infrared 0103 physical sciences Drug Discovery Molecule Physical and Theoretical Chemistry Triplet state infrared spectroscopy 010303 astronomy & astrophysics ComputingMilieux_MISCELLANEOUS media_common Physics Photons 010304 chemical physics helium chemistry Organic Chemistry Observable Hydrogen atom early universe Universe [CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] TheoryofComputation_MATHEMATICALLOGICANDFORMALLANGUAGES Chemistry (miscellaneous) Quantum Theory Molecular Medicine [PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph] Software Hydrogen |
Zdroj: | Molecules, Vol 25, Iss 2183, p 2183 (2020) Molecules Molecules, MDPI, 2020, 25 (9), pp.2183. ⟨10.3390/molecules25092183⟩ Volume 25 Issue 9 |
ISSN: | 1420-3049 |
DOI: | 10.3390/molecules25092183 |
Popis: | HeHHe + is the only potential molecule comprised of atoms present in the early universe that is also easily observable in the infrared. This molecule has been known to exist in mass spectrometry experiments for nearly half-a-century and is likely present, but as-of-yet unconfirmed, in cold plasmas. There can exist only a handful of plausible primordial molecules in the epochs before metals (elements with nuclei heavier than 4 He as astronomers call them) were synthesized in the universe, and most of these are both rotationally and vibrationally dark. The current work brings HeHHe + into the discussion as a possible (and potentially only) molecular candle for probing high-z and any metal-deprived regions due to its exceptionally bright infrared feature previously predicted to lie at 7.43 &mu m. Furthermore, the present study provides new insights into its possible formation mechanisms as well as marked stability, along with the decisive role of anharmonic zero-point energies. A new entrance pathway is proposed through the triplet state ( 3 B 1 ) of the He 2 H + molecule complexed with a hydrogen atom and a subsequent 10.90 eV charge transfer/photon emission into the linear and vibrationally-bright 1 &Sigma g + HeHHe + form. |
Databáze: | OpenAIRE |
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