scholarly journals Nonadiabatic decay of Rydberg-atom–ion molecules

2022 ◽  
Vol 105 (1) ◽  
Author(s):  
A. Duspayev ◽  
G. Raithel
Keyword(s):  
2021 ◽  
Vol 2 ◽  
pp. 1-13
Author(s):  
Charles T. Fancher ◽  
David R. Scherer ◽  
Marc C. St. John ◽  
Bonnie L. Schmittberger Marlow

2020 ◽  
Vol 9 (5) ◽  
pp. 305-312
Author(s):  
Ryan Cardman ◽  
Luís F. Gonçalves ◽  
Rachel E. Sapiro ◽  
Georg Raithel ◽  
David A. Anderson

AbstractWe present electric field measurements and imaging of a Yagi–Uda antenna near-field using a Rydberg atom–based radio frequency electric field measurement instrument. The instrument uses electromagnetically induced transparency with Rydberg states of cesium atoms in a room-temperature vapor and off-resonant RF-field–induced Rydberg-level shifts for optical SI-traceable measurements of RF electric fields over a wide amplitude and frequency range. The electric field along the antenna boresight is measured using the atomic probe at a spatial resolution of ${\lambda }_{RF}/2$ with electric field measurement uncertainties below 5.5%, an improvement to RF measurement uncertainties provided by existing antenna standards.


2011 ◽  
Vol 20 (4) ◽  
Author(s):  
Anatolij A. Mihajlov ◽  
Ljubinko M. Ignjatović ◽  
Vladimir A. Srécković ◽  
Milan S. Dimitrijević

AbstractThe chemi-ionization processes in atom - Rydberg atom collisions, as well as the corresponding chemi-recombination processes, are considered as factors of influence on the atom exited-state populations in weakly ionized layers of stellar atmospheres. The presented results are related to the photospheres of the Sun and some M red dwarfs, as well as weakly ionized layers of DB white dwarf atmospheres. It has been found that the mentioned chemi-ionization and recombination processes dominate over the concurrent electron-atom and electron-ion ionization and recombination processes in all parts of the considered stellar atmospheres. The obtained results demonstrate the fact that the considered processes must have significant influence on the optical properties of stellar atmospheres. It is shown that these processes and their importance for non-local thermodynamic equilibrium (non-LTE) modeling of the solar atmospheres should be investigated further.


2018 ◽  
Vol 26 (9) ◽  
pp. 12330 ◽  
Author(s):  
Yi-Mou Liu ◽  
Xue-Dong Tian ◽  
Jing Wang ◽  
Chu-Hui Fan ◽  
Feng Gao ◽  
...  

2003 ◽  
Vol 68 (2) ◽  
pp. C44-C47 ◽  
Author(s):  
F B Dunning ◽  
C O Reinhold ◽  
J Burgdorfer

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