A Theoretical Study for the Valence−Rydberg Interaction in Diatomic Molecules. Application to the NO β Band System-Reference-Cited by-同舟云学术

A Theoretical Study for the Valence−Rydberg Interaction in Diatomic Molecules. Application to the NO β Band System

Published:2004-11-24 Issue:51 Volume:108 Page:11279-11284
ISSN:1089-5639
Container-title:The Journal of Physical Chemistry A
language:en
Short-container-title:J. Phys. Chem. A

Author:

Bustos E.¹,Granucci G.¹,Persico M.¹,Velasco A. M.¹,Martín I.¹,Lavín C.¹

Affiliation:

1. Departamento de Química Física y Química Inorgánica, Facultad de Ciencias, Universidad de Valladolid, E-47005 Valladolid, Spain, and Dipartimento di Chimica e Chimica Industriale, Università di Pisa, I-56126 Pisa, Italy

Publisher

American Chemical Society (ACS)

Subject

Physical and Theoretical Chemistry

Link

https://pubs.acs.org/doi/pdf/10.1021/jp046924g

Reference31 articles.

1. Oscillator Strengths in the Far Ultraviolet. I. Nitric Oxide

2. Hasson, V.; Nicholls, R. W.J. Phys. B: At. Mol. Opt. Phys.1971,4, 1769.

3. Absolute oscillator strength estimates for some bands of the β-system of nitric oxide

4. NO(B 2Π) radiative lifetimes: v=0–6

5. Electronic transition moment variation and Einstein coefficients for the NO(B 2Π–X 2Π) system

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