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Phys. Rev. A 68, 032722 (2003) [6 pages]

Pressure shift and broadening of the 254-nm intercombination line of mercury by N2

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James P. Jacobs
Department of Physics and Astronomy, University of Montana, Missoula, Montana 59812, USA

R. Bruce Warrington*
Department of Physics, FM-15, University of Washington, Seattle, Washington 98195, USA

Received 4 June 2003; published 29 September 2003

We have used laser absorption spectroscopy to study the collisional broadening and shift of the 254-nm 61S0→63P1 intercombination line of Hg in the presence of N2 for pressures below 400 Torr. This study comprises the first measurements of the proportionality constants for pressure broadening and shift of Hg due to N2 in this pressure range, and the first high-precision measurements of these pressure effects on Hg for any foreign gas. We obtain -2.54(2)MHz/Torr for the shift and 9.01(4) MHz/Torr for the broadening (full width at half maximum) at 21°C (95% confidence interval). These results are important for ongoing experiments using optical pumping of mercury in tests of fundamental symmetries, as well as for characterization of interatomic forces and tests of the theory of collisional line broadening.

© 2003 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.68.032722
DOI:
10.1103/PhysRevA.68.032722
PACS:
34.20.-b, 32.70.Jz, 39.30.+w

*Present address: CSIRO Telecommunications and Industrial Physics, P. O. Box 218, Lindfield NSW 2070, Sydney, Australia.