rotational level
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2022 ◽  
Author(s):  
Helen Chadwick ◽  
Mark Somers ◽  
Aisling Stewart ◽  
Yosef Alkoby ◽  
Thomas Carter ◽  
...  

Abstract Rotational motion lies at the heart of intermolecular, molecule-surface chemistry and cold molecule science, motivating the development of methods to excite and de-excite rotations. Existing schemes involve perturbing the molecules with photons or electrons which supply or remove energy comparable to the rotational level spacing. Here, we study the possibility of de-exciting the molecular rotation of a D2 molecule, from a J=2 to the non-rotating J=0 state, without using an energy-matched perturbation. We show that a magnetic field which splits the rotational projection states by only pico eV, can change the probability that a molecule-surface collision will stop a molecule from rotating and lose rotational energy which is 9 orders larger than that of the magnetic manipulation. Calculations confirm the origin of the control scheme, but also underestimate rotational flips (Δm_J≠0), highlighting the importance of the results as a sensitive benchmark for further developing theoretical models of molecule-surface interactions.


Author(s):  
Christian Balança ◽  
Ernesto Quintas-Sánchez ◽  
Richard Dawes ◽  
Fabien Dumouchel ◽  
François Lique ◽  
...  

Abstract Carbon-chain anions were recently detected in the interstellar medium. These very reactive species are used as tracers of the physical and chemical conditions in a variety of astrophysical environments. However, the Local Thermodynamical Equilibrium conditions are generally not fulfilled in these environments. Therefore, collisional as well as radiative rates are needed to accurately model the observed emission lines. We determine in this work the state-to-state rate coefficients of C4H− in collision with both ortho- and para-H2. A new ab initio 4D potential energy surface was computed using explicitly-correlated coupled cluster procedures. This surface was then employed to determine rotational excitation and de-excitation cross sections and rate coefficients for the first 21 rotational levels (up to rotational level j1 = 20) using the close-coupling method, while the coupled-state approximation was used to extend the calculations up to j1 = 30. State-to-state rate coefficients were obtained for the temperature range 2–100 K. The differences between the ortho- and para-H2 rate coefficients are found to be small.


2020 ◽  
Author(s):  
◽  
Casey D. Foley

Decades of experimental and theoretical achievements built on the foundations of thermochemistry and quantum mechanics have birthed the field of molecular dynamics where intimate details of individual reactive events can be mapped. On the ground state of formaldehyde, two dissociation pathways are commonly known, one proceeding over a high barrier through a three-center, tight transition state to give molecular products, and another via homolytic simple bond fission to radical products. A third, distinct ground state dissociation pathway first seen in formaldehyde 15 years ago, the 'roaming' mechanism, involves incipient radicals, but the H atom samples a large, flat region of the PES, roaming in the van der Waals region, leading to an intramolecular H + HCO reaction. Roaming reactions have been visualized from a classical perspective with only a few exceptions in the literature despite the likely quantum nature of the process. A major objective of the presented work is to reveal quantum aspects of roaming reactions. Here, a few different molecules (C3H3Cl, HDCO, and H2CO) were investigated with the goal of characterizing roaming radicals on the ground state, where roaming observations have primarily occurred. Knowledge of the excited states of propargyl chloride was necessary to understand the experimental observations from investigation of its ground state. Ultraviolet (UV) photodissociation and state-specific detection with velocity map imaging of Cl, Cl*, and C3H3 were interpreted with the aid of multireference calculations to characterize the nature of the electronic excitations. A series of triplet states were identified to preferentially dissociate to Cl or Cl*. Infrared multiphoton excitation and infrared multiphoton dissociation (IRMPD) of propargyl chloride enhanced UV processes and allowed for radical dissociation at threshold. IRMPD on the ground state produced HCl following isomerization to 1-chloroallene, where a roaming-like transition state with Cl in an abstraction geometry is adopted. Accurate H and D atom ground state radical thresholds of singly deuterated formaldehyde, HDCO, were obtained from velocity map imaging to aid future studies HDCO dynamics studies. The different radical thresholds, arising from the difference in zero-point energies, is a purely quantum phenomenon. PHOFEX spectra over a wide range were collected, creating a library of known frequencies of rotational lines that can be used to study the dynamics of different vibrational bands and the energy dependence of different processes. Heats of formation of HDCO and DCO were also determined. Finally, a detailed examination of the photochemical dynamics in both ortho and para nuclear spin isomers of formaldehyde is provided, exploring the full range of parent rotational levels from J = 0 to 4, initially prepared via excitation of specific rotational lines of a range of vibrational bands on the first singlet excited state (2141, 2161, 2143, 2241, 2243). Measurements of the entire CO (v = 0) product rotational distributions are combined with velocity map imaging of selected CO product states to obtain a complete picture of the photochemical dynamics for each specific parent rotational level. Distributions are found to vary dramatically with small changes in total energy, effects not captured at all by classical treatments. Full quantum state correlations reveal interactions among three formaldehyde dissociation continua, yielding rich insight into the dynamics of this highly excited molecule as it decays to products. An orbiting resonance dominates the dynamics, though other possible dynamical phenomena are noted.


2020 ◽  
Vol 20 (9) ◽  
pp. 5269-5292 ◽  
Author(s):  
Stefan Noll ◽  
Holger Winkler ◽  
Oleg Goussev ◽  
Bastian Proxauf

Abstract. OH airglow is an important nocturnal emission of the Earth's mesopause region. As it is chemiluminescent radiation in a thin medium, the population distribution over the various roto-vibrational OH energy levels of the electronic ground state is not in local thermodynamic equilibrium (LTE). In order to better understand these non-LTE effects, we studied hundreds of OH lines in a high-quality mean spectrum based on observations with the high-resolution Ultraviolet and Visual Echelle Spectrograph at Cerro Paranal in Chile. Our derived populations cover vibrational levels between v=3 and 9, rotational levels up to N=24, and individual Λ-doublet components when resolved. As the reliability of these results critically depends on the Einstein-A coefficients used, we tested six different sets and found clear systematic errors in all of them, especially for Q-branch lines and individual Λ-doublet components. In order to minimise the deviations in the populations for the same upper level, we used the most promising coefficients from Brooke et al. (2016) and further improved them with an empirical correction approach. The resulting rotational level populations show a clear bimodality for each v, which is characterised by a probably fully thermalised cold component and a hot population where the rotational temperature increases between v=9 and 4 from about 700 to about 7000 K, and the corresponding contribution to the total population at the lowest N decreases by an order of magnitude. The presence of the hot populations causes non-LTE contributions to rotational temperatures at low N, which can be estimated quite robustly based on the two-temperature model. The bimodality is also clearly indicated by the dependence of the populations on changes in the effective emission height of the OH emission layer. The degree of thermalisation decreases with increasing layer height due to a higher fraction of the hot component. Our high-quality population data are promising with respect to a better understanding of the OH thermalisation process.


2019 ◽  
Author(s):  
Stefan Noll ◽  
Holger Winkler ◽  
Oleg Goussev ◽  
Bastian Proxauf

Abstract. OH airglow is an important nocturnal emission of the Earth's mesopause region. As it is chemiluminescent radiation in a thin medium, the population distribution over the various roto-vibrational OH energy levels of the electronic ground state is not in local thermodynamic equilibrium (LTE). In order to better understand these non-LTE effects, we studied hundreds of OH lines in a high-quality mean spectrum based on observations with the high-resolution Ultraviolet and Visual Echelle Spectrograph at Cerro Paranal in Chile. Our derived populations cover vibrational levels between v = 3 and 9, rotational levels up to N = 24, and individual Λ-doublet components when resolved. As the reliability of these results critically depends on the Einstein-A coefficients used, we tested six different sets and found clear systematic errors in all of them, especially for Q-branch lines and individual Λ-doublet components. In order to minimise the deviations in the populations for the same upper level, we used the most promising coefficients from Brooke et al. (2016, JQSRT 168, 142) and further improved them with an empirical correction approach. The resulting rotational level populations show a clear bimodality for each v, which is characterised by a probably fully thermalised cold component and a hot population where the rotational temperature increases between v = 9 and 4 from about 700 to about 7,000 K and the corresponding contribution to the total population at the lowest N decreases by an order of magnitude. The presence of the hot populations causes non-LTE contributions to rotational temperatures at low N, which can be estimated quite robustly based on the two-temperature model. The bimodality is also clearly indicated by the dependence of the populations on changes in the effective emission height of the OH emission layer. The degree of thermalisation decreases with increasing layer height due to a higher fraction of the hot component. Our high-quality population data are promising with respect to a better understanding of the OH thermalisation process.


2019 ◽  
Vol 488 (4) ◽  
pp. 4732-4739 ◽  
Author(s):  
Maxence Lepers ◽  
Grégoire Guillon ◽  
Pascal Honvault

ABSTRACT We use the time-independent quantum-mechanical formulation of reactive collisions in order to investigate the state-to-state H+ + HD → D+ + H2 chemical reaction. We compute cross-sections for collision energies up to 1.8 eV and rate coefficients for temperatures up to 10 000 K. We consider HD in the lowest vibrational level v = 0 and rotational levels j = 0–6, and H2 in vibrational levels v′ = 0–3 and rotational levels j′ = 0–9. For temperatures below 4000 K, the rate coefficients strongly vary with the initial rotational level j, depending on whether the reaction is endothermic (j ≤ 2) or exothermic (j ≥ 3). The reaction is also found less and less probable as the final vibrational quantum number v′ increases. Our results illustrate the importance of studying state-to-state reactions, in the context of the chemistry of the primordial universe.


2017 ◽  
Vol 55 (2) ◽  
pp. 165-173 ◽  
Author(s):  
V. M. Atrazhev ◽  
V. A. Shakhatov ◽  
R. E. Boltnev ◽  
N. Bonifaci ◽  
F. Aitken ◽  
...  

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