TY - JOUR
T1 - Velocity Map Imaging Spectroscopy of the Dipole-Bound State of CH2CN-
T2 - Implications for the Diffuse Interstellar Bands
AU - Laws, Benjamin A.
AU - Levey, Zachariah D.
AU - Schmidt, Timothy W.
AU - Gibson, Stephen T.
N1 - Publisher Copyright:
©
PY - 2021/11/10
Y1 - 2021/11/10
N2 - Weakly bound anionic systems present a new domain for negative ion spectroscopy. Here we report on a multifaceted study of the CH2CN- dipole-bound state, employing high-resolution photoelectron spectroscopy from 130 different wavelengths, velocity-map imaging at threshold, and laser scanning photodetachment experiments. This uncovers a wide variety of different vibrational and rotational autodetaching resonances. By examination of both sides of the problem, absorption from the anion to the dipole-bound state and vibrational/rotational autodetachment to the neutral, a complete model of the dipole-bound chemistry is formed. Precise values for the electron affinity EA = 12468.9(1) cm-1, dipole binding energy DBE = 40.2(3) cm-1, and anion inversion splitting ω5 = 115.9(2) cm-1 are obtained. This model is then employed to study possible astronomical implications, revealing good agreement between the K = 1 ← 0 CH2CN- dipole transition and the λ8040 diffuse interstellar band.
AB - Weakly bound anionic systems present a new domain for negative ion spectroscopy. Here we report on a multifaceted study of the CH2CN- dipole-bound state, employing high-resolution photoelectron spectroscopy from 130 different wavelengths, velocity-map imaging at threshold, and laser scanning photodetachment experiments. This uncovers a wide variety of different vibrational and rotational autodetaching resonances. By examination of both sides of the problem, absorption from the anion to the dipole-bound state and vibrational/rotational autodetachment to the neutral, a complete model of the dipole-bound chemistry is formed. Precise values for the electron affinity EA = 12468.9(1) cm-1, dipole binding energy DBE = 40.2(3) cm-1, and anion inversion splitting ω5 = 115.9(2) cm-1 are obtained. This model is then employed to study possible astronomical implications, revealing good agreement between the K = 1 ← 0 CH2CN- dipole transition and the λ8040 diffuse interstellar band.
UR - http://www.scopus.com/inward/record.url?scp=85119261025&partnerID=8YFLogxK
U2 - 10.1021/jacs.1c08762
DO - 10.1021/jacs.1c08762
M3 - Article
SN - 0002-7863
VL - 143
SP - 18684
EP - 18692
JO - Journal of the American Chemical Society
JF - Journal of the American Chemical Society
IS - 44
ER -