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1.
The reactions of the lowest metastable states of Ar, Kr and Xe with XeF2 were studied in a flowing afterglow apparatus; XeF emission (from D2Π12 and B 2Π+ states) was observed in all cases. The total rate constants (cm3 molecule?1 s?1) for XeF* formation were determined as 75 × 10?11 ? Xe(3P2);64 × 10?11 ? Kr(3P2) and 20 × 10?11 ? Ar(3P0,2). The reactions of Ar(3P0,2) and Kr(3P2) with XeF2 also gave ArF* and KrF*, respectively. Analysis of these emissions indicates that at least two different mechanisms are operative: reactive quenching by the ionic—covalent curve-crossing mechanism and excitation transfer. The Ar(3P0,2 + XeF2 reaction is a sufficiently strong source of XeF(D—X) emission that the main features of the XeF(D2Π12 ? X2Σ+) system could be photographed and tentative assignments of these vibrational bands are given. The XeF(D → B) emission could not be observed and the ratio of the D—X versus the D—B transition probability must be > 1000 : 1.  相似文献   

2.
Mercury 63P0 metastables were shown to sensitize the emission of a number of diatomic free radicals (HgH, HgCl, CN, OH, and NH) of photochemical interest. Evidence is presented that the energy transfer process is a non-Franck-Condon one at least for HgCl and CN. An inverse rotational temperature dependence on nitrogen pressure was observed for the HgH(2Π12) u′ = 0 state and attributed to near resonant rotational-rotational relaxation processes involving the zeroth and first vibrational levels.  相似文献   

3.
The ESR method is used to study the oxidation kinetics of the CH3, C2H5, n-C4H9, i-C4H9, s-C4H9, t-C4H9, n-C6H13, C6H11, C6H5CH2, CH3C6H4CH2, and C6H5CH2CH2 radicals in methanol matrix at 87 K. The reaction kinetics are shown to be describable in terms of a time-dependent rate constant k(t). The contribution from the matrix relaxation to k(t) has been determined. The oxidation rate and the shape of the kinetic curve are independent of the type of the radical. Models interpreting the experimental data are discussed.  相似文献   

4.
The electronic energy transfer process Hg(6 3P0) + OH(X2Πi, υ = 0,K) → Hg(6 1S0) + OH(A 2Σ+, υ,K) has been studied by the sensitized fluorescence method. A rather broad spectrum of rotational population, Nυ′K, was obtained under conditions of minimum relaxation, which illustrates the non-resonant and non-optical nature of this energy transfer process. The fractions of the exoergicity, above electronic excitation of OH(A 2Σ+, υ = 0, K = 0), going into vibrational, rotational and translational excitation are 0.11, 0.31, and 0.58, respectively. A statistical mode of energy partitioning, such as would result from long-lived complex formation, seems to account well for these observations.  相似文献   

5.
A simple method is described for studying the reactions of metastable Ar(3P0) and Ar(3P2) atoms separately in a discharge-flow system. CO and Kr quench these states with rate constants in the ratio k0 (CO)/k2 (CO) = 8±1 and k2 (Kr)/k0(Kr) = 18±2.  相似文献   

6.
The excitation-transfer reaction in thermal energy collisions of state-selected metastable Ar*(3P2) and Ar*(3P0) atoms with ground state H atoms, giving excited H*(n = 2) atoms, has been studied with the stationary afterglow technique. The rate constant for the excitation of H atoms by Ar*(3P2) has been found to be more than one order of magnitude larger than in excitation by Ar*(3P0). This difference in the reactivity of two metastable species is explained to be a consequence of the attractive nature of the D(2II) and E(2Σ+) potentials that develop from the Ar*(3P2)+H entrance channel and which give curve crossing with the B(2II) and C(2Σ+ potentials, respectively, leading to the Ar+H*(n=2) exit channel, whereas only a repulsive 4II (Ω=12) potential develops from the Ar*(3P0+H entrance channel.  相似文献   

7.
Photobromination of SiH4 under uv-irradiation at various wavelengths has been studied. Rate constants for the elementary reactions Br(2P3/2)+SiH4HBr+SiH3 (k=3.2×10–11 exp(–21.8±2.5)/RT, cm3/s) and Br* (2P1/2)+SiH4HBr+SiH3 (k*=(3±1)×10–13 cm3/s) have been determined in the temperature range from 300 to 415 K.
- . Br(2P3/2)+SiH4HBr+SiH3, k=3,2×10–11 exp (–21,8±2,5)/RT 3/ Br*(2P1/2)+SiH4HBr+SiH3, k*=(3±1)×10–13 3/ 300–415 K.
  相似文献   

8.
The vibrational analysis of the CN(B2Σ+ → X2Σ+) emission sensitized by Hg(63P0) metastables has shown that the energy transfer process, Hg(63P0) + CN(X2Σ+) → Hg(61S0) + CN(B2Σ+), populates the CN(B2Σ+) state in a non-Franck-Condon fashion. The relative vibrational populations for the ν = 0 to 4 states are 1.00, 0.56 ± 0.06, 0.26 ± 0.03, 0.11 ± 0.03 and 0.04 ± 0.01, respectively. Long-range attractive interaction between the Hg(63P0) atom and the CN(X2Σ+) radical is evidenced by the observed high rotational excitation of the CN(B2Σ+) radical following the energy transfer process.  相似文献   

9.
The gas phase reactions of Ge(3P0,1) and Si(3PJ) with O2, NO and N2O have been studied in a flow tube system at 350 K. Atomic Ge and Si were produced by flowing GeH4 and SiH4 through a hollow cathode discharge. The subsequent disappearance of the Ge and Si atoms was followed with atomic absorption spectroscopy. Rate constants were determined for the reactions at 4 and 5 torr pressures.  相似文献   

10.
A comparative spectroscopic study in the visible and ultraviolet ranges was conducted on the flowing afterglows resulting from the reactions of He(2 3S) and Ne(3P0,2) metastables with CS2. Penning ionization was found to be the predominant energy transfer process. However, electron—ion recombination within the afterglows constitutes a major secondary process and gives rise to the most intense emitting system, CS(A 1 Π → X 1Σ+). Both afterglows were found to produce the CS+2(B2Σ+u-X2Πg), CS+2(A2Πu-X2Πg) and CS(a 3Π-X 1Σ+) emission systems as well as some atomic sulfur emission lines. Some intensity differences were observed and are interpreted in terms of energetics and the formation mechanisms of the emitting species. A moderately strong CS+(A 2Πi-X 2Σ+) emission system was also observed in the ehlium afterglow. In addition, a weak, sharp group of bands in the 390–420 nm range in the helium afterglow has been determined to be due to the presence of a small amount of He+ ions. This group of bands consists of two overlapping emission systems and are identified as CS(B 1Σ+ → A 1Π) and CS+(B 2Σ+ → A 2Πi).  相似文献   

11.
Absolute cross sections for the quenching of Cd(5 3P1 and Cd(5 3P0) by carbon monoxide, carbon dioxide and nitric oxide have been determined by a phase-shift method. It was found that carbon monoxide deactivates the Cd3P1) atoms not only to the ground state, Cd(1S0), but also to the metastable state, Cd(3P0), and that the cross section for the latter process is ten times larger than that for the former one. On the contrary, carbon dioxide quenches Cd(3P1) atoms to the 1S0 state without producing Cd(3P0) atoms. The quenching efficiency by nitric oxide was considerably large compared with those of carbon mono- and di-oxides. These quenching cross sections were compared with those of other excited metal atom states.  相似文献   

12.
Photon-echo quantum beats observed in the two-pulse and three-pulse photon echo of the 3P03H4 transition in Pr3+/LaF3 were used to determine the excited-state spin-hamiltonian. In addition we report on the anomalous stimulated photon echo observed in the same transition which in a magnetic field may acquire a lifetime of about 30 minutes.  相似文献   

13.
Energy-transfer reactions between He(2 3S) and Ne(3P0.2) metastable atoms and PN radicals have been investigated by emission spectroscopy. Thirteen new PN+ (B 1Σ+ ?X 2Σ+) emission bands were found in addition to eight previously identified bands in the range 305–395 nm. From these observed band-head wavelengths, the following molecular constants were obtained for the X and B states of PN+ : PN+ (X): ωc = 1306 ± 3 cm?1, ωcxc = 7.9 ± 0.7 cm?1, PN? (B): Tc = 31354 ± 6 cm?1, ωc = 719 ± 3 cm?1, ωcxc = 1.6 ± 0.7 cm?1. The PN+ (B) state vibrational population was estimated from the emission intensities and the calculated Morse Franck—Condon (FC) factors for the PN+ (B–X) transition. Both the results obtained by He(2 3S) and Ne(3P0.2) Penning ionization shifted to lower vibrational levels in comparison with the calculated FC factors for vertical PN(X) → PN+ (B) ionization. Besides PN+ (B–X) emission, unidentified bands were observed in the 231–236 nm region in the helium afterglow, probably originating from PN or PN?.  相似文献   

14.
New global three dimensional potential energy surfaces for the Cl+H2 reactive system have been constructed using accurate multireference configuration interaction calculations with a large basis set. The three lowest adiabatic potential energy surfaces correlating asymptotically with Cl(^2p)+H2 have been transformed to adiabatic representation, which leads to a fourth coupling potential for non-linear geometries. In addition, the spin-orbit coupling surfaces have also been computed using the Breit-Pauli Hamiltonian. Properties of the new potential are described. Reaction dynamics based on the new potential agrees with the recent experimental results quite well.  相似文献   

15.
In this work we studied the collinear F(2 P 1/2) + H2 system in a strong CO2 laser field. It was found that the trajectory. surface hopping method (TSHM) yields entirely different results than the exact quantum-mechanical treatment. A curvecrossing model was devised to explain the discrepancy.  相似文献   

16.
The photochlorination of methyl fluoride has been studied at low pressures. Excited (2P1/2) chlorine atoms have been found to participate in the reaction. The ratio of the excited and ground state rate constants has been estimated at room temperature.
. (2P1/2) . .
  相似文献   

17.
Vacuum UV emission from the products of quenching ofAr(3Po) and Ar(3P2) by several reagents has been compared. The large differences suggest that Ar(3Po) and Ar(3P2) preferentially yield respectively the D(12) and B(12) excited states of ArBr or ArCl, which show specific, but very different, predissociation patterns.  相似文献   

18.
The chemiluminescent interaction of Xe(3P2,0) and BrCN has been studied under crosscd-beam conditions at collision energies ranging up to 70 kj mol?1. The CN(B → X) fluorescence spectrum, the excitation function for its production and the fluorescence polarisation - or rather its absence - have been determined. The results can be explained by a two-stage harpooning mechanism involving an inert-gas cyanide (Xe+CN?)1 intermediate but not by a “sensitisation” mechanism proceeding through electronic energy transfer.  相似文献   

19.
The ultraviolet luminescence from the Hg-photosensitised reaction of ammonia was investigated at pressures up to 10 atmospheres. From a variation of the wavelength distribution on the [NH3], it was concluded that Hg(63P0) can attach clusters of NH3 molecules to form Hg(NH3)n* with n up to at least 5. The emission profiles of the stabilized complexes with n = 1–4 were determined, and also the profile from unstabilised HgNH3* formed in a bimolecular encounter of Hg(63P0) with NH3. Dissociation constants for complexes with n = 2, 3 and 4 were measured.  相似文献   

20.
Steady-state and transient photokinetic and spectroscopic measurements on aqueous Eu(NO3)3 show different affinities of 7F, 5D1 and 5D0 Eu3+aq towards nitrate ion. This may be rationalised by differences in the inner- and outer-shell hydration structures between 5DO, 5D1 Eu3+(aq) and 7F Eu3+(aq). Nitrate penetration into the inner-shell of Eu3+(aq), and inner-coordination (EuNO2+3)* exciplex formation, occur solely in the long-lived 5DO level of Eu3+(aq).  相似文献   

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