The Quenching of Mercury Resonance Radiation (2537A) by Nitrogen
- 1 November 1953
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 92 (3) , 637-641
- https://doi.org/10.1103/physrev.92.637
Abstract
When a mercury atom in the resonance state collides with a nitrogen molecule, it may be transferred to the metastable state. The cross section for this reaction has been measured by a new method. Mercury vapor, in the presence of a known pressure of nitrogen gas, is excited by 2537A radiation. After the source of the excitation is cut off, the decay time of the imprisoned radiation is observed. The quenching collision cross section is calculated from the measured decay time and the known value of the imprisonment time in the absence of the quenching gas. Measurements have been taken over the temperature range 325-525°K; is found to increase from 5.0× at the lower temperature to 1.0× at the upper temperature.
Keywords
This publication has 9 references indexed in Scilit:
- New Developments in the Production and Measurement of Ultra High VacuumJournal of Applied Physics, 1953
- Isotope Effect in the Imprisonment of Resonance RadiationPhysical Review B, 1952
- Imprisonment of Resonance Radiation in Gases. IIPhysical Review B, 1951
- A Null-Reading Absolute ManometerReview of Scientific Instruments, 1951
- Imprisonment of Resonance Radiation in Mercury VaporPhysical Review B, 1949
- Imprisonment of Resonance Radiation in GasesPhysical Review B, 1947
- The Quenching of Mercury Resonance Radiation by Hydrogen, Carbon Monoxide and NitrogenPhysical Review B, 1934
- Effects of Temperature and Nitrogen Pressure on the Afterglow of Mercury Resonance RadiationPhysical Review B, 1932
- New Experimental Determination of Effective Cross-Sections for the Quenching of Mercury Resonance RadiationPhysical Review B, 1930