Subpromille Measurements and Calculations of CO (3-0) Overtone Line Intensities.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
22 Jul 2022
Historique:
received: 16 03 2022
accepted: 26 05 2022
entrez: 8 8 2022
pubmed: 9 8 2022
medline: 11 8 2022
Statut: ppublish

Résumé

Intensities of lines in the near-infrared second overtone band (3-0) of ^{12}C^{16}O are measured and calculated to an unprecedented degree of precision and accuracy. Agreement between theory and experiment to better than 1‰ is demonstrated by results from two laboratories involving two independent absorption- and dispersion-based cavity-enhanced techniques. Similarly, independent Fourier transform spectroscopy measurements of stronger lines in this band yield mutual agreement and consistency with theory at the 1‰ level. This set of highly accurate intensities can provide an intrinsic reference for reducing biases in future measurements of spectroscopic peak areas.

Identifiants

pubmed: 35939021
doi: 10.1103/PhysRevLett.129.043002
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

043002

Auteurs

Katarzyna Bielska (K)

Institute of Physics, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziadzka 5, 87-100 Torun, Poland.

Aleksandra A Kyuberis (AA)

Van Swinderen Institute for Particle Physics and Gravity, University of Groningen, Nijenborgh 4, 9747AG Groningen, The Netherlands.

Zachary D Reed (ZD)

Chemical Sciences Division, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA.

Gang Li (G)

PTB (Physikalisch-Technische Bundesanstalt), Bundesallee 100, 38116 Braunschweig, Germany.

Agata Cygan (A)

Institute of Physics, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziadzka 5, 87-100 Torun, Poland.

Roman Ciuryło (R)

Institute of Physics, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziadzka 5, 87-100 Torun, Poland.

Erin M Adkins (EM)

Chemical Sciences Division, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA.

Lorenzo Lodi (L)

Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom.

Nikolay F Zobov (NF)

Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom.

Volker Ebert (V)

PTB (Physikalisch-Technische Bundesanstalt), Bundesallee 100, 38116 Braunschweig, Germany.

Daniel Lisak (D)

Institute of Physics, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziadzka 5, 87-100 Torun, Poland.

Joseph T Hodges (JT)

Chemical Sciences Division, National Institute of Standards and Technology, Gaithersburg, Maryland 20899, USA.

Jonathan Tennyson (J)

Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom.

Oleg L Polyansky (OL)

Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom.

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Classifications MeSH