Infra-red chemiluminescence I. Infra-red emission from hydrogen chloride formed in the systems atomic hydrogen plus chlorine, atomic hydrogen plus hydrogen chloride, atomic hydrogen plus deuterium chloride, and atomic deuterium plus hydrogen chloride

Infra-red emission arising from several room-temperature gas-phase reactions has previously been described by the authors in preliminary communications (Cashion & Polanyi 1958, 1959 a, b, c ). In the present work, details of this new technique are given. Spectra obtained from the systems H + Cl 2 , H + HCl, H + DCl and D + HCl are described. These consist of the resolved spectra of the HCl fundamental transitions (∆ v = 1) in the ground electronic state, the partially resolved first overtones (∆ v = 2) and, in one system, the unresolved second overtones (∆ v = 3). The system H + Cl 2 gives rise to emission from all vibrational levels up to and including v = 6; the system H + HCl from all levels up to and including v = 7. A detailed examination of the spectra obtained from the systems H + HCl, H + DCl and D + HCl leads to the conclusion that these emissions arise from the formation of vibrationally excited HCl or DCl as the product of an association reaction between hydrogen atoms and chlorine atoms (in the presence of some ‘third body’, M ). This result constitutes the first direct evidence for the view that association reactions lead to the formation of highly vibrating molecules (Polanyi 1959). Also consistent with this view is the observation made here that HCl or DCl acting as a third body in association reactions is not excited to levels higher than v = 1. The bulk of the emission observed from the system H + Cl 2 is believed to arise from the exchange reaction H + Cl 2 = HClꜛ v ≼ 6 + Cl (where HClꜛ is vibrationally excited HCl in its ground electronic state). The vibrational distribution of HClꜛ in the system H + Cl 2 , under our experimental conditions, conforms approximately to a Boltzmann distribution for a vibrational temperature of 2700°K. From this observed distribution a calculation of the initial distribution is made, which would indicate that the HClꜛ are formed initially in all accessible vibrational levels, lower levels being favoured over higher. However, this result is based on the arbitrary assumption that vibrational-vibrational exchange between HClꜛ molecules is negligible. The distribution of HClꜛ among rotational levels of v = 1 in the system H + Cl 2 is definitely non-Boltzmann. The excess rotational energy over room temperature equilibrium energy, is shown to come from an even greater excess present in the HClꜛ as originally formed. The absolute intensity of the emission is calculated at ca . 0.005 W. It is estimated that roughly 1 to 10 % of the heat of reaction goes into vibrational excitation.

The flash photolysis of cyanogen, cyanogen bromide and cyanogen iodide has been studied under isothermal conditions. Vibrationally excited (v” ⩽ 6) cyanogen radicals were produced and observed spectroscopically in absorption, in the δ v = 0, ± 1 and — 2 sequences of the violet ( B 2 ∑ ← X 2 ∑) system. The CN radical produced in the reaction CN R + hv → CN( X 2 ∑, v = 0) + R is excited electronically, CN( X 2 ∑, v = 0)+ hv → CN ( B 2 ∑, v = 0, 1, 2, ...), and then returns to various vibrational levels of the ground state by fluorescence or collision CN( B 2 ∑, v = 0, 1, 2, ...) → CN( X 2 ∑, v = 0, 1, 2, ...) + hv , CN( B 2 ∑, v = 0, 1, 2, ...) + M → CN( X 2 ∑, v = 0, 1, 2, ...) + M . Frequent repetition of this type of excitation in the absence of relaxation would lead to a vibrational ‘tem perature’ which may be described as virtually infinite, and in any case is extremely high when relaxation is relatively slow. The alternative reactions by which vibrationally excited radicals could be produced, namely CN R + hv → CN( X 2 ∑, v ⩽ 6) + R and CN R + hv → CN( A 2 II , v > 0) + R , followed by CN( A 2 II , v > 0) → CN( X 2 ∑, v > 0), were shown to account for < 6 % of the vibrationally excited radicals observed and may be entirely inoperative. The probability of energy transfer to CNBr from the fourth vibrational level of CN, P 4-3 , was found to be approximately 1 × 10 -2 . The rate constant for the recombination of cyanogen radicals at room temperature was found to be ~ 6 x 10 11 ml. mole -1 s -1 or ~ 1.7 × 10 16 ml. 2 mole -2 s -1 with nitrogen as third body.


1960 ◽  
Vol 38 (10) ◽  
pp. 1742-1755 ◽  
Author(s):  
P. E. Charters ◽  
J. C. Polanyi

A multiple reflection apparatus for the observation of infrared chemiluminescence is described. By means of this apparatus infrared emission from the system H + O2 has been identified as being due to vibrationally excited OH radicals in levels v = 1, 2, and 3 of the ground electronic state. The resolved infrared spectrum of the OH fundamental has been observed for the first time without interference from other emission. The most likely source of excited OH is the reaction H + HO2 → OH† + OH. The vibrational 'temperature' of OH† (vibrationally excited OH in its ground electronic state) in our system is in the region of TV = 2240 °K. These findings are discussed in relation to Krassovsky's suggestion that reaction between H and O2 could account for the Meinel hydroxyl bands in the night sky.


2015 ◽  
Vol 17 (16) ◽  
pp. 10478-10488 ◽  
Author(s):  
Florian Ehlers ◽  
Mirko Scholz ◽  
Jens Schimpfhauser ◽  
Jürgen Bienert ◽  
Kawon Oum ◽  
...  

The S* signal of carotenoids corresponds to vibrationally hot molecules in the ground electronic state S0*.


AIP Advances ◽  
2015 ◽  
Vol 5 (9) ◽  
pp. 097101 ◽  
Author(s):  
M. Zervos ◽  
C. Mihailescu ◽  
J. Giapintzakis ◽  
A. Othonos ◽  
A. Travlos

2020 ◽  
Vol 22 (42) ◽  
pp. 24257-24269 ◽  
Author(s):  
Attila Tajti ◽  
Péter G. Szalay ◽  
Roman Kochanov ◽  
Vladimir G. Tyuterev

The accuracy of variationally calculated vibrational levels of ozone can be greatly improved by adding diagonal Born–Oppenheimer correction to the best available ab initio potential.


The photolytic decomposition of ozone in ultra-violet radiation has been studied by kinetic spectroscopy. It has been shown that vibrationally excited oxygen in its ground electronic state plays a most important part in the decomposition. These molecules have sufficient vibrational energy to bring about dissociation of ozone, thus regenerating oxygen atoms which can again produce vibrationally excited oxygen. The importance of this energy chain is emphasized by comparative studies on the explosive decomposition of pure ozone, and the isothermal decomposition when an excess of inert gas is present. In the former case the O* 2 is removed so rapidly, mainly by reaction with ozone, that no absorption due to it can be detected. Using an excess of inert gas to obtain isothermal conditions it has been possible to observe Schumann–Runge absorption of oxygen molecules in their ground electronic state, with up to 16 quanta of vibrational energy. The vibrational energy distribution of the oxygen molecules formed has an apparent maximum at v " = 13 (53.5 kcal/mole) and falls off sharply at v " = 12 and 16 (49.0 and 63.2 kcal/mole). It is shown that the only reasonable reaction for the production of excited oxygen is O + O 3 → O* 2 + O 2 . Studies on the rate of ozone decay with time have also been carried out and the results analyzed in terms of the rate constants of reactions involving the deactivation of excited oxygen and the three-body recombination O + O 2 + M → O 3 + M . It is shown that the spherically symmetrical and chemically inert gases such as A, He and SF 6 are much less efficient in bringing about recombination than N 2 , N 2 O or CO 2 .


1995 ◽  
Vol 103 (13) ◽  
pp. 5864-5867 ◽  
Author(s):  
Kenneth A. Cowen ◽  
K. Thomas Lorenz ◽  
Yu‐Fong Yen ◽  
Michael F. Herman ◽  
Brent Koplitz

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