Abstract

This paper calculates the potential energy curves of the 14 Λ-S and 49 Ω states, which come from the first three dissociation channels of the SiN− anion. These calculations are conducted using the valence internally contracted multireference configuration interaction and the Davidson correction approach. Core-valence correlation and scalar relativistic corrections are taken into account. The potential energies are extrapolated to the complete basis set limit. The spin-orbit coupling is computed using the state interaction approach with the Breit–Pauli Hamiltonian. We found that the X1Σ+ (υ′′ = 0–23) and a3Σ+ (υ′ = 0–2) states of SiN− are stable at the computed adiabatic electron affinity value of 23,262.27 cm−1 for SiN. Based on the calculated potential energy curves, the spectroscopic parameters and vibrational levels were determined for all stable and metastable Λ-S and Ω states. The computed adiabatic electron affinity of SiN and the spectroscopic constants of SiN− (X1Σ+) are all in agreement with the available experimental data. The d3Σ+, 25Σ+, 15Δ, and 15Σ− quasi-bound states caused by avoided crossings were found. Calculations of the transition dipole moment of a3Σ+1 to X1Σ+0+ are shown. Franck-Condon factors, Einstein coefficients, and radiative lifetimes of the transition from the a3Σ+1 (υ′ = 0–2) to the X1Σ+0+ state are evaluated.

Highlights

  • SiN− is analogous with the known interstellar CN− anion [1]

  • 2 show the potential energy curve (PEC) of 14 electronic states obtained by the internally contracted multireference configuration interaction (icMRCI) + Q/56 + CV + DK

  • Employing the PECs determined by the icMRCI + Q/56 + CV + DK calculations, we evaluated the spectroscopic parameters of 13 Λ-S states

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Summary

Introduction

SiN− is analogous with the known interstellar CN− anion [1]. Several silicon-containing nitrogen chains (SiN, SiCN, and SiNC) have been detected in the interstellar medium [2,3,4]. Kerkines and Mavridis [15] in 2005 calculated the spectroscopic constants and energetics for the SiN (X2 Σ+ , A2 Π) and SiN− (X1 Σ+ , a3 Σ+ ) at the level of the theory of the restricted coupled-cluster method with all singles and doubles and noniterative inclusion of triples [RCCSD(T)]. Their best estimated AEA is 24,212.75 cm−1. The spectroscopic parameters, vibrational levels, and transition probabilities obtained here can be considered very reliable

Methodology
Λ-S states
Electron Affinity of SiN
Spectroscopic Parameters and Vibrational Levels of the 45 Ω Bound States
Spectroscopic and Vibrational Properties of 16 Ω States with the Σ Symmetry
Spectroscopic and Vibrational Properties of 20 Ω States with the Π Symmetry
Transition
Asrange with of theinternuclear
TDMs versus internuclear separations ofoftransitions
Conclusions
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