RT info:eu-repo/semantics/article
T1 Theoretical Study of the Rotational Structure of the c4′1Σu                  + (6)–X1Σg                  +(0–9) Absorption Bands of N2
A1 Alonso, J. L.
A1 Redondo Cristóbal, María del Pilar
A1 Velasco Sanz, Ana María
A1 Lavín Puente, María del Carmen
K1 Molecular spectroscopy (2095); Line intensities (2084); Radiative processes (2055)
K1 Line intensities (2084)
K1 Radiative processes (2055)
AB We have theoretically determined the absorption oscillator strengths and wavenumbers for rotationally resolved transitions of the c4′1Σu + (6)-X1Σg +(0–9) bands of N2, which are relevant to analyze the spectra of planetary atmospheres. The Molecular Quantum Defect Orbital method has been used in our calculations. The interaction between the c4′1Σu + (6) Rydberg state and the b′1Σu + valence states has been considered using an adequate rovibronic energy matrix. In addition, we have calculated the lifetimes of the rotational levels of the c4′1Σu + (6) state. We hope that the reported data, most of them for the first time, can be useful in the interpretation of planetary atmospheres where N2 is present.
PB American Astronomical Society
SN 0004-637X
YR 2021
FD 2021
LK https://uvadoc.uva.es/handle/10324/64757
UL https://uvadoc.uva.es/handle/10324/64757
LA spa
NO The Astrophysical Journal, 922:100 (9pp), 2021 December 1
NO Producción Científica
DS UVaDOC
RD 24-dic-2024