The Possible Interstellar Anion CH2CN-: Spectroscopic Constants, Vibrational Frequencies, and Other Considerations
arXiv:1305.1660 · doi:10.1088/0004-637X/762/2/121
Abstract
It is hypothesized that the A ^1B_1 <- X ^1A' excitation into the dipole-bound state of the cyanomethyl anion (CH2CN-) is proposed as the carrier for one diffuse interstellar band. However, this particular molecular system has not been detected in the interstellar medium even though the related cyanomethyl radical and the isoelectronic ketenimine molecule have been found. In this study we are employing the use of proven quartic force fields and second-order vibrational perturbation theory to compute accurate spectroscopic constants and fundamental vibrational frequencies for ^1A' CH2CN- in order to assist in laboratory studies and astronomical observations.
References in corpus (4)
Cited by in corpus (9)
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- Singlet Excited States of Anions with Higher Main Group Elements
- Electronic and Rovibrational Quantum Chemical Analysis of CP: The Next Interstellar Anion?
- Spectroscopic characteristics of the cyanomethyl anion and its deuterated derivatives
- Theoretical Electronic and Rovibrational Studies for Anions of Interest to the DIBs
- The Fundamental Vibrational Frequencies and Spectroscopic Constants of the Dicyanoamine Anion, NCNCN (CN): Quantum Chemical Analysis for Astrophysical and Planetary Environments
- Observation of a core-excited dipole-bound state 1 eV above the electron detachment threshold in cryogenically cooled acetylacetonate