Theoretical study of the g factor and lifetime of the 6s6 p P-3(0) state of mercury
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Authors
Porsev, S. G.
Safronova, U. I.
Safronova, M. S.
Issue Date
2017
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Article
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Abstract
We calculate the g factor of the 6s6p (3) P-0 state of 199 and 201 mercury isotopes using a relativistic high-precision all-order method that combines the configuration interaction and the coupled-cluster approaches. Our values g(Hg-199) = -0.9485(49) x 10(-3) and g(Hg-201) = 0.3504(18) x 10(-3) are in agreement with the experimental measurements within the 0.5% theoretical uncertainty. We also calculate the hyperfine quenching rate of the 6s6p P-3(0) state in Hg-199 and Hg-201 and determine its lifetime to be 1.3 and 1.9 s, respectively.
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Porsev, S. G., Safronova, U. I., & Safronova, M. S. (2017). Theoretical study of the g factor and lifetime of the 6s6pP03 state of mercury. Physical Review A, 96(1). doi:10.1103/physreva.96.012509
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In Copyright (All Rights Reserved)
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2469-9926