High-resolution vacuum-ultraviolet and ultraviolet photoionization spectroscopy of krypton
Year: 2002
Authors: Brandi F., Hogervorst W., Ubachs W.
Autors Affiliation: Laser Centre, Department of Physics and Astronomy, Vrije Universiteit, De Boelelaan 1081, 1081 HV Amsterdam, Netherlands
Abstract: Accurate spectroscopy of krypton is performed on five transitions from the (4p(6)) (1)S(0) ground state to the 5d[1/2](1), 6s[3/2](1), 5p[1/2](0), 5p[3/2](2) and 5p[5/2](2) excited states (jl-coupling notation) by means of 1VUV + 1UV and 2UV + 1UV resonance-enhanced photoionization. Isotope shifts of all six stable isotopes are determined, and a King plot analysis indicates a large field shift factor even for transitions in which no s electron is involved. Absolute frequency calibration is performed on three transitions, leading to a novel determination of the excited state energies of Kr with an accuracy of similar to0.0013 cm(-1). An accurate value for the ionization energy of (86)Kr, 112 914.516(14) cm(-1), is derived along with ionization energies for all even isotopes. The ac Stark effect on the two-photon transition to the 5p[1/2](0) excited state is investigated. For light intensities up to similar to260 MW cm(-2) a linear shift of 0.75(48) Hz (W cm(-2))(-1) is observed, while at higher intensities the line exhibits a sub-linear shift and an asymmetric broadening. Consequences of the results obtained for the 5p[1/2]0 state on resonance-enhanced narrow-band XUV/VUV generation are discussed.
Journal/Review: JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS
Volume: 35 (4) Pages from: 1071 to: 1084
KeyWords: OPTICAL FREQUENCY CALIBRATION; REFERENCE IODINE LINES; LASER-SPECTROSCOPY; ISOTOPE SHIFTS; RYDBERG SERIES; ENERGY-LEVELS; krypton
DOI: 10.1088/0953-4075/35/4/329ImpactFactor: 1.969Citations: 38data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2024-11-24References taken from IsiWeb of Knowledge: (subscribers only)Connecting to view paper tab on IsiWeb: Click hereConnecting to view citations from IsiWeb: Click here