High-precision isotope-shift measurement of23S-23Ptransition in helium

1991 ◽  
Vol 66 (5) ◽  
pp. 592-595 ◽  
Author(s):  
Ping Zhao ◽  
J. R. Lawall ◽  
F. M. Pipkin
1991 ◽  
Author(s):  
Ping Zhao ◽  
J. R. Lawall ◽  
F. M. Pipkin

2019 ◽  
Vol 44 (14) ◽  
pp. 3462
Author(s):  
Bin Wang ◽  
Weifeng Zhang ◽  
Xinyu Fan ◽  
Jianping Yao

1997 ◽  
Author(s):  
Yi-qun Lu ◽  
Ma Jun ◽  
J. S. Zhang ◽  
Y. C. Zhang ◽  
M. G. Gao ◽  
...  

2003 ◽  
Vol 76 (3) ◽  
pp. 209-213 ◽  
Author(s):  
K. Matsubara ◽  
U. Tanaka ◽  
H. Imajo ◽  
S. Urabe ◽  
M. Watanabe

1965 ◽  
Vol 7 (12) ◽  
pp. 322-324 ◽  
Author(s):  
R. H. Cordover ◽  
T. S. Jaseja ◽  
A. Javan

2019 ◽  
Vol 29 (04) ◽  
pp. 1940005 ◽  
Author(s):  
Ming-Sheng Zhan ◽  
Jin Wang ◽  
Wei-Tou Ni ◽  
Dong-Feng Gao ◽  
Gang Wang ◽  
...  

The Zhaoshan long-baseline Atom Interferometer Gravitation Antenna (ZAIGA) is a new type of underground laser-linked interferometer facility, and is currently under construction. It is in the 200-m-on-average underground of a mountain named Zhaoshan which is about 80[Formula: see text]km southeast to Wuhan. ZAIGA will be equipped with long-baseline atom interferometers, high-precision atom clocks, and large-scale gyros. ZAIGA facility will take an equilateral triangle configuration with two 1-km-apart atom interferometers in each arm, a 300-m vertical tunnel with atom fountain and atom clocks mounted, and a tracking-and-ranging 1-km-arm-length prototype with lattice optical clocks linked by locked lasers. The ZAIGA facility will be used for experimental research on gravitation and related problems including gravitational wave detection, high-precision test of the equivalence principle of micro-particles, clock-based gravitational red-shift measurement, rotation measurement and gravitomagnetic effect.


1988 ◽  
Vol 66 (7) ◽  
pp. 586-611 ◽  
Author(s):  
G. W. Drake

The unified method described previously for combining high-precision nonrelativistic variational calculations with relativistic and quantum electrodynamic corrections is applied to the 1s2 1S0, 1s2s 1S0, 1s2s 3S1, 1s2p 1P1, and 1s2p 3P0,1,2 staters of helium-like ions. Detailed tabulations are presented for all ions in the range 2 ≤ Z ≤ 100 and are compared with a wide range of experimental data up to 34Kr+. The results for 90U+ significantly alter the recent Lamb shift measurement of Munger and Gould from 70.4 ± 8.3 to 71.0 ± 8.3 eV, in comparison with a revised theoretical value of 74.3 ± 0.4 eV. The improved agreement is due to the inclusion of higher order two-electron corrections in the present work.


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