Chemi-ionization processes

1993 ◽  
Vol 163 (6) ◽  
pp. 39 ◽  
Author(s):  
A.N. Klucharev
Keyword(s):  
2019 ◽  
Vol 0 (9) ◽  
pp. 9-14
Author(s):  
A. V. Ushakov ◽  
◽  
I. V. Karpov ◽  
L. Yu. Fedorov ◽  
E.A. Dorozhkina ◽  
...  

2017 ◽  
Vol 31 (29) ◽  
pp. 1750215 ◽  
Author(s):  
Feras Afaneh ◽  
Horst Schmidt-Böcking

In this paper, we study single and double ionizations of N2O in a short elliptically polarized 800 nm laser pulse using the COLTRIMS technique. The molecular-frame photoelectron angular distribution and the ion sum-momentum distribution of single and double ionizations of N2O molecules are reported for the single ionization dissociative channel NO[Formula: see text] + N and the double ionization dissociative channel NO[Formula: see text] + N[Formula: see text]. The ionizations of multiple orbitals for the two studied dissociative channels were identified via studying the orientation dependent ionization rates for their KERs. The results show that the shape of the ionizing orbitals governs the single and double ionization processes of N2O.


2021 ◽  
Vol 11 (1) ◽  
Author(s):  
Hua Shu ◽  
Jiangtao Li ◽  
Yucheng Tu ◽  
Junjian Ye ◽  
Junyue Wang ◽  
...  

AbstractThe sound velocities of water in the Hugoniot states are investigated by laser shock compression of precompressed water in a diamond anvil cell. The obtained sound velocities in the off-Hugoniot region of liquid water at precompressed conditions are used to test the predictions of quantum molecular dynamics (QMD) simulations and the SESAME equation-of-state (EOS) library. It is found that the prediction of QMD simulations agrees with the experimental data while the prediction of SESAME EOS library underestimates the sound velocities probably due to its improper accounting for the ionization processes.


1998 ◽  
Vol 176 (3) ◽  
pp. 189-201 ◽  
Author(s):  
Kéiko Hattori ◽  
T.James S. Cole ◽  
Douglas P. Menagh

Author(s):  
Irina V. Beregovaya ◽  
Irina S. Tretyakova ◽  
Vsevolod I. Borovkov

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.


1974 ◽  
Vol 52 (3) ◽  
pp. 359-364 ◽  
Author(s):  
Peter F. Carr ◽  
Patricia Christensen ◽  
Derek E. Wilson ◽  
David A. Armstrong

The ionization yield from fast electron impact on DCl under radiolysis conditions at 200 to 650 Torr was found to be 1.006 ± 0.023 times that from HCl. Also primary ionization processes were investigated by mass spectrometry. The relative abundance of Cl+ from HCl near threshold at 17.4 eV was about twice that from DCl, but processes with onset at and above 21.0 eV did not exhibit an isotope effect. The interpretation of the results and their implications concerning the mechanism of radiolysis of HCl were discussed.


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