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Molecular N2 emission, observed from an Ar(3Po, 2) and Xe(3P2) + N2 flowing afterglow apparatus, indicates that the energy pooling reaction by 2N2(A 3Σ+u) generates the emission from the Herman infrared system, which is an unassigned nitrogen band system. A lower limit to the formation rate constant for the upper state of the Herman infrared system was found to be 2.5 × 10-11 cm3 molecule?1 s?1. The information presented here may help in the identification of the upper and lower states of the emission system. The 2N2(A) energy pooling reaction also forms N2(B3 Πg, v? 8) but a rate constant cannot be assigned from the present data.  相似文献   
2.
We report X 1A' and 2 1A' potential energy surfaces for HCN. Thermal isomerisation on the ground-state surface is discussed. An avoided crossing between X 1A' and 2 1A' suggests alternative isomerisation mechanisms via this excited state. The X1A'-21A' interaction may also allow the formation of CN(X 2Σ+) in photodissociation of XCN molecules.  相似文献   
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