scholarly journals Angular momentum distribution in Rydberg states excited by a strong laser pulse

2018 ◽  
Vol 98 (4) ◽  
Author(s):  
J. Venzke ◽  
R. Reiff ◽  
Z. Xue ◽  
A. Jaroń-Becker ◽  
A. Becker
2021 ◽  
Vol 6 (3) ◽  
pp. 034401
Author(s):  
A. S. Samsonov ◽  
I. Yu. Kostyukov ◽  
E. N. Nerush

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.


1969 ◽  
Vol 136 (2) ◽  
pp. 465-480 ◽  
Author(s):  
J.O. Rasmussen ◽  
W. Nörenberg ◽  
H.J. Mang

Nanoscale ◽  
2017 ◽  
Vol 9 (34) ◽  
pp. 12391-12397 ◽  
Author(s):  
Franco P. Bonafé ◽  
Bálint Aradi ◽  
Mengxue Guan ◽  
Oscar A. Douglas-Gallardo ◽  
Chao Lian ◽  
...  

We report the first real-time computational study that shows evidence of sub-picosecond beathing oscillations in metal nanoparticles under strong laser pulse illumination.


2009 ◽  
Vol 5 (S265) ◽  
pp. 420-421
Author(s):  
João A. S. Amarante ◽  
Helio J. Rocha-Pinto

AbstractWe investigate the angular momentum distribution of known exoplanetary systems, as a function of the planetary mass, orbital semimajor axis and metallicity of the host star. We find exoplanets seems to be classified according to at least two ‘populations’, with respect to their angular momentum properties. This classification is independent on the composition of the planet and seems to be valid for both jovian and neptunian planets, and probably can be extrapolated to the terrestrial planets of the Solar System. We analyse these ‘populations’ considering the phenomenon of planetary migration.


Sign in / Sign up

Export Citation Format

Share Document