Oscillator strengths and line widths of dipole-allowed transitions in ¹⁴N₂ between 89.7 and 93.5 nm
| dc.contributor.author | Stark, G. | |
| dc.contributor.author | Lewis, B. R. | |
| dc.contributor.author | Heays, Alan | |
| dc.contributor.author | Yoshino, K. | |
| dc.contributor.author | Smith, P. L. | |
| dc.contributor.author | Ito, K. | |
| dc.date.accessioned | 2015-11-23T05:23:27Z | |
| dc.date.available | 2015-11-23T05:23:27Z | |
| dc.date.issued | 2008-03-17 | |
| dc.date.updated | 2015-12-09T07:26:39Z | |
| dc.description.abstract | Line oscillator strengths in the 20 electric dipole-allowed bands of ¹⁴N₂ in the 89.7–93.5nm (111480–106950cm⁻¹) region are reported from photoabsorptionmeasurements at an instrumental resolution of ∼6mÅ (0.7cm⁻¹) full width at half maximum. The absorptionspectrum comprises transitions to vibrational levels of the 3pσᵤc′₄¹Σᵤ⁺, 3pπᵤc³Πᵤ, and 3sσgo₃¹ΠᵤRydberg states and of the b′¹Σᵤ⁺ and b¹Πᵤ valence states. The J dependences of band f values derived from the experimental line f values are reported as polynomials in J′(J′+1) and are extrapolated to J′=0 in order to facilitate comparisons with results of coupled Schrödinger-equation calculations. Most bands in this study are characterized by a strong J dependence of the band f values and display anomalous P-, Q-, and R-branch intensity patterns. Predissociation line widths, which are reported for 11 bands, also exhibit strong J dependences. The f value and line width patterns can inform current efforts to develop comprehensive spectroscopic models that incorporate rotational effects and predissociation mechanisms, and they are critical for the construction of realistic atmospheric radiative-transfer models. | |
| dc.description.sponsorship | This work was supported in part by NASA Grant No. NNG05GA03G to Wellesley College and Australian Research Council Discovery Program Grant No. DP0558962. | en_AU |
| dc.identifier.issn | 0021-9606 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/16618 | |
| dc.publisher | American Institute of Physics (AIP) | |
| dc.relation | http://purl.org/au-research/grants/arc/DP0558962 | |
| dc.rights | http://www.sherpa.ac.uk/romeo/issn/0021-9606..."Publishers version/PDF may be used on author's personal website, institutional website or institutional repository" from SHERPA/RoMEO site (as at 23/11/15). Copyright 2008 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in The Journal of Chemical Physics and may be found at https://doi.org/10.1063/1.2834933 | |
| dc.source | The Journal of Chemical Physics | |
| dc.subject | Keywords: Absorption; Electric dipole moments; Polynomials; Rydberg states; Spectroscopic analysis; Spectrum analysis; Photoabsorption; Predissociation mechanisms; Oscillators (electronic) | |
| dc.title | Oscillator strengths and line widths of dipole-allowed transitions in ¹⁴N₂ between 89.7 and 93.5 nm | |
| dc.type | Journal article | |
| local.bibliographicCitation.issue | 11 | en_AU |
| local.bibliographicCitation.lastpage | 10 | |
| local.bibliographicCitation.startpage | 114302 | en_AU |
| local.contributor.affiliation | Stark, Glenn, Wellesley College, United States of America | en_AU |
| local.contributor.affiliation | Lewis, Brenton, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Atomic and Molecular Physics Laboratories, The Australian National University | en_AU |
| local.contributor.affiliation | Heays, Alan, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Atomic and Molecular Physics Laboratories, The Australian National University | en_AU |
| local.contributor.affiliation | Yoshino, K, Harvard-Smithsonian Center for Astrophysics, United States of America | en_AU |
| local.contributor.affiliation | Smith, P.L., Harvard-Smithsonian Center for Astrophysics, United States of America | en_AU |
| local.contributor.affiliation | Ito, K., High Energy Accelerator Research Organization (Photon Factory), Japan | en_AU |
| local.contributor.authoruid | u7901135 | en_AU |
| local.description.notes | Imported from ARIES | en_AU |
| local.identifier.absfor | 020201 | en_AU |
| local.identifier.ariespublication | u4169254xPUB169 | en_AU |
| local.identifier.citationvolume | 128 | en_AU |
| local.identifier.doi | 10.1063/1.2834933 | en_AU |
| local.identifier.scopusID | 2-s2.0-41149171377 | |
| local.identifier.thomsonID | 000254292500022 | |
| local.publisher.url | https://www.aip.org/ | en_AU |
| local.type.status | Published Version | en_AU |
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