scholarly journals Highly charged ions for atomic clocks and search for variation of the fine structure constant

2015 ◽  
Vol 236 (1-3) ◽  
pp. 79-86 ◽  
Author(s):  
V. A. Dzuba ◽  
V. V. Flambaum
1995 ◽  
Vol 74 (18) ◽  
pp. 3511-3514 ◽  
Author(s):  
John D. Prestage ◽  
Robert L. Tjoelker ◽  
Lute Maleki

2018 ◽  
Vol 4 (12) ◽  
pp. eaau4869 ◽  
Author(s):  
P. Wcisło ◽  
P. Ablewski ◽  
K. Beloy ◽  
S. Bilicki ◽  
M. Bober ◽  
...  

We report on the first Earth-scale quantum sensor network based on optical atomic clocks aimed at dark matter (DM) detection. Exploiting differences in the susceptibilities to the fine-structure constant of essential parts of an optical atomic clock, i.e., the cold atoms and the optical reference cavity, we can perform sensitive searches for DM signatures without the need for real-time comparisons of the clocks. We report a two orders of magnitude improvement in constraints on transient variations of the fine-structure constant, which considerably improves the detection limit for the standard model (SM)–DM coupling. We use Yb and Sr optical atomic clocks at four laboratories on three continents to search for both topological defect and massive scalar field candidates. No signal consistent with a DM coupling is identified, leading to considerably improved constraints on the DM-SM couplings.


2020 ◽  
Vol 22 (9) ◽  
pp. 093010 ◽  
Author(s):  
B M Roberts ◽  
P Delva ◽  
A Al-Masoudi ◽  
A Amy-Klein ◽  
C Bærentsen ◽  
...  

2019 ◽  
Vol 10 (1) ◽  
Author(s):  
H. Bekker ◽  
A. Borschevsky ◽  
Z. Harman ◽  
C. H. Keitel ◽  
T. Pfeifer ◽  
...  

AbstractRecent theoretical works have proposed atomic clocks based on narrow optical transitions in highly charged ions. The most interesting candidates for searches of physics beyond the Standard Model are those which occur at rare orbital crossings where the shell structure of the periodic table is reordered. There are only three such crossings expected to be accessible in highly charged ions, and hitherto none have been observed as both experiment and theory have proven difficult. In this work we observe an orbital crossing in a system chosen to be tractable from both sides: Pr$${}^{9+}$$9+. We present electron beam ion trap measurements of its spectra, including the inter-configuration lines that reveal the sought-after crossing. With state-of-the-art calculations we show that the proposed nHz-wide clock line has a very high sensitivity to variation of the fine-structure constant, $$\alpha$$α, and violation of local Lorentz invariance; and has extremely low sensitivity to external perturbations.


1984 ◽  
Vol 86 ◽  
pp. 151-153
Author(s):  
J.F. Seely ◽  
U. Feldman ◽  
G.A. Doschek

The measurement of transition energies in highly charged ions represents an important test of quantum electrodynamics (QED) in strong fields. The OED contributions to the hydrogenic transition energies increase as (αZ)4, where α is the fine structure constant and Z is the atomic number. Transitions in hydrogenic ions of sulfur, chlorine, argon, and iron have previously been measured to a precision of 100 ppm or better. These measurements are in satisfactory agreement with accurate calculations of the energy levels, and this confirms the calculation of the QED contributions to the energy levels of one-electron ions.


Symmetry ◽  
2020 ◽  
Vol 12 (3) ◽  
pp. 344
Author(s):  
T. D. Le

Astrophysical tests of current values for dimensionless constants known on Earth, such as the fine-structure constant, α , and proton-to-electron mass ratio, μ = m p / m e , are communicated using data from high-resolution quasar spectra in different regions or epochs of the universe. The symmetry wavelengths of [Fe II] lines from redshifted quasar spectra of J110325-264515 and their corresponding values in the laboratory were combined to find a new limit on space-time variations in the proton-to-electron mass ratio, ∆ μ / μ = ( 0.096 ± 0.182 ) × 10 − 7 . The results show how the indicated astrophysical observations can further improve the accuracy and space-time variations of physics constants.


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