scholarly journals Isomer-specific vibronic structure of the 9-, 1-, and 2-anthracenyl radicals via slow photoelectron velocity-map imaging

2016 ◽  
Vol 113 (7) ◽  
pp. 1698-1705 ◽  
Author(s):  
Marissa L. Weichman ◽  
Jessalyn A. DeVine ◽  
Daniel S. Levine ◽  
Jongjin B. Kim ◽  
Daniel M. Neumark

Polycyclic aromatic hydrocarbons, in various charge and protonation states, are key compounds relevant to combustion chemistry and astrochemistry. Here, we probe the vibrational and electronic spectroscopy of gas-phase 9-, 1-, and 2-anthracenyl radicals (C14H9) by photodetachment of the corresponding cryogenically cooled anions via slow photoelectron velocity-map imaging (cryo-SEVI). The use of a newly designed velocity-map imaging lens in combination with ion cooling yields photoelectron spectra with <2 cm−1 resolution. Isomer selection of the anions is achieved using gas-phase synthesis techniques, resulting in observation and interpretation of detailed vibronic structure of the ground and lowest excited states for the three anthracenyl radical isomers. The ground-state bands yield electron affinities and vibrational frequencies for several Franck–Condon active modes of the 9-, 1-, and 2-anthracenyl radicals; term energies of the first excited states of these species are also measured. Spectra are interpreted through comparison with ab initio quantum chemistry calculations, Franck–Condon simulations, and calculations of threshold photodetachment cross sections and anisotropies. Experimental measures of the subtle differences in energetics and relative stabilities of these radical isomers are of interest from the perspective of fundamental physical organic chemistry and aid in understanding their behavior and reactivity in interstellar and combustion environments. Additionally, spectroscopic characterization of these species in the laboratory is essential for their potential identification in astrochemical data.

2019 ◽  
Author(s):  
Mark Babin ◽  
Jessalyn DeVine ◽  
John F. Stanton ◽  
Daniel Neumark ◽  
Martin DeWitt

<p></p><p>High-resolution anion photoelectron spectra of cryogenically cooled NO<sub>3</sub>ˉ anions obtained using slow photoelectron velocity-map imaging are presented and provide new insight into the vibronic structure of the corresponding neutral radical. A combination of improved spectral resolution, measurement of energy-dependent intensity effects, temperature control, and comparison to theory allows for full assignment of the vibronic features observed in this spectrum. We obtain a refined electron affinity of 3.9289(14) eV for NO<sub>3</sub>. Further, the appearance of Franck-Condon forbidden transitions from vibrationally cold anions to neutral states with excitation along the NO<sub>3</sub> <i>v</i><sub>4</sub> mode confirms that these features arise from vibronic coupling with the excited state of NO<sub>3</sub> and are not hot bands as has been suggested. Together, the suite of experimental and simulated results provides clear evidence that the <i>v</i><sub>3</sub> fundamental of NO<sub>3</sub> resides near 1050 cm<sup>−1</sup>, addressing a long-standing controversy surrounding this vibrational assignment.</p> <p> </p><br><p></p>


2019 ◽  
Author(s):  
Mark Babin ◽  
Jessalyn DeVine ◽  
John F. Stanton ◽  
Daniel Neumark ◽  
Martin DeWitt

<p></p><p>High-resolution anion photoelectron spectra of cryogenically cooled NO<sub>3</sub>ˉ anions obtained using slow photoelectron velocity-map imaging are presented and provide new insight into the vibronic structure of the corresponding neutral radical. A combination of improved spectral resolution, measurement of energy-dependent intensity effects, temperature control, and comparison to theory allows for full assignment of the vibronic features observed in this spectrum. We obtain a refined electron affinity of 3.9289(14) eV for NO<sub>3</sub>. Further, the appearance of Franck-Condon forbidden transitions from vibrationally cold anions to neutral states with excitation along the NO<sub>3</sub> <i>v</i><sub>4</sub> mode confirms that these features arise from vibronic coupling with the excited state of NO<sub>3</sub> and are not hot bands as has been suggested. Together, the suite of experimental and simulated results provides clear evidence that the <i>v</i><sub>3</sub> fundamental of NO<sub>3</sub> resides near 1050 cm<sup>−1</sup>, addressing a long-standing controversy surrounding this vibrational assignment.</p> <p> </p><br><p></p>


2019 ◽  
Vol 217 ◽  
pp. 235-255 ◽  
Author(s):  
Jessalyn A. DeVine ◽  
Mark C. Babin ◽  
Daniel M. Neumark

High-resolution photoelectron spectroscopy of cryogenically-cooled aluminum oxide anions shows new subtleties in the vibronic structure of Al2O2−/0 and Al3O3−/0.


2013 ◽  
Vol 9 (S297) ◽  
pp. 265-275
Author(s):  
F. Huisken ◽  
G. Rouillé ◽  
M. Steglich ◽  
Y. Carpentier ◽  
C. Jäger ◽  
...  

AbstractThe electronic spectroscopy of various polycyclic aromatic hydrocarbon (PAH) molecules has been studied in the laboratory at low temperatures using both molecular beam and matrix isolation spectroscopy techniques. While molecular beam spectra can be readily compared to astronomical observations, the band positions measured in Ne and Ar matrices are extrapolated to obtain rather good estimates for the same transitions in the gas phase. Absolute absorption cross sections are determined for gas-phase and matrix spectra by comparing them with calibrated solution spectra. All laboratory results are analyzed and discussed in view of the role that PAHs can play as carriers of the diffuse interstellar bands (DIBs). Our studies suggest that regular neutral PAHs are not responsible for any of the known strong DIBs.


2019 ◽  
Author(s):  
Marta L. Vidal ◽  
Anna Krylov ◽  
Sonia Coriani

We report on the implementation and illustrative applications of Dyson orbitals within the recently proposed frozen-core (fc) core-valence separated (CVS) equation-of-motion (EOM) coupled-cluster singles and doubles (CCSD) method, which enables efficient and accurate characterization of core-ionized states. Dyson orbitals are reduced quantities that can be interpreted as correlated states of the ejected/attached electron.<br>Dyson orbitals enter the expressions of various experimental observables, such as photoionization cross sections; thus, they are necessary for modeling photoelectron spectra.<br>Here we discuss the simulations of X-ray photoelectron spectra (XPS) and propose an approach to simulate time-resolved (TR-)XPS for probing excited states. <br>As illustrative examples, we present the simulation of the XPS of the ground state of adenine and of TR-XPS of the excited states of uracil.


Author(s):  
Kelly Chance ◽  
Randall V. Martin

This chapter provides a broad overview of the spectroscopic principles required in order to perform quantitative spectroscopy of atmospheres. It couples the details of atmospheric spectroscopy with the radiative transfer processes and also with the assessment of rotational, vibrational, and electronic spectroscopic measurements of atmospheres. The principles apply from line-resolved measurements (chiefly microwave through infrared) through ultraviolet and visible measurements employing absorption cross sections developed from individual transitions. The chapter introduces Einstein coefficients before in turn discussing rotational spectroscopy, vibrational spectroscopy, nuclear spin, and electronic spectroscopy.


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