A self‐consistent multiple‐peak structure of the photoemission spectra of metallic Fe 2 p as a function of film thickness

2020 ◽  
Vol 52 (9) ◽  
pp. 591-599
Author(s):  
Alberto Herrera‐Gomez ◽  
Orlando Cortazar‐Martínez ◽  
Jesus‐Fernando Fabian‐Jocobi ◽  
Abraham Carmona‐Carmona ◽  
Joaquin‐Gerardo Raboño‐Borbolla ◽  
...  
1997 ◽  
Vol 08 (05) ◽  
pp. 1145-1158
Author(s):  
J. J. Rodríguez-Núñez ◽  
S. Schafroth

We implement the numerical method of summing Green function diagrams on the Matsubara frequency axis for the fluctuation exchange (FLEX) approximation. Our method has previously been applied to the attractive Hubbard model for low density. Here we apply our numerical algorithm to the Hubbard model close to half filling (ρ =0.40), and for T/t = 0.03, in order to study the dynamics of one- and two-particle Green functions. For the values of the chosen parameters we see the formation of three branches which we associate with the two-peak structure in the imaginary part of the self-energy. From the imaginary part of the self-energy we conclude that our system is a Fermi liquid (for the temperature investigated here), since Im Σ( k , ω) ≈ w2 around the chemical potential. We have compared our fully self-consistent FLEX solutions with a lower order approximation where the internal Green functions are approximated by free Green functions. These two approches, i.e., the fully self-consistent and the non-self-consistent ones give different results for the parameters considered here. However, they have similar global results for small densities.


2010 ◽  
Vol 107 (12) ◽  
pp. 123520 ◽  
Author(s):  
Yan Kai Xu ◽  
Sadao Adachi

1984 ◽  
Vol 89 (A10) ◽  
pp. 9101 ◽  
Author(s):  
R. D. Belian ◽  
D. N. Baker ◽  
E. W. Hones ◽  
P. R. Higbie

2010 ◽  
Vol 19 (04) ◽  
pp. 558-567 ◽  
Author(s):  
V. O. NESTERENKO ◽  
J. KVASIL ◽  
P. VESELY ◽  
W. KLEINIG ◽  
P.-G. REINHARD

The self-consistent separable random-phase approximation (SRPA) with Skyrme forces is extended to the case of magnetic excitations and applied to the description of spin-flip and orbital M1 giant resonances in the isotopic chain 142-152 Nd . The Skyrme forces SkT6, SkM*, SLy6 and SkI3 are used. The calculations show an onset of the scissors mode with increasing deformation. A specific three-peak structure of the spin-flip response is found and explained by particular neutron and proton spin-flip transitions. Although the employed forces provide an acceptable qualitative description, the Skyrme functional still needs further improvement to reproduce quantitatively the experiment for spin modes.


2013 ◽  
Vol 113 (4) ◽  
pp. 044312
Author(s):  
Shai Levy ◽  
Issai Shlimak ◽  
David H. Dressler ◽  
Tiecheng Lu

1999 ◽  
Vol 173 ◽  
pp. 37-44
Author(s):  
M.D. Melita ◽  
A. Brunini

AbstractA self-consistent study of the formation of planetary bodies beyond the orbit of Saturn and the evolution of Kuiper disks is carried out by means of an N-body code where accretion and gravitational encounters are considered. This investigation is focused on the aggregation of massive bodies in the outer planetary region and on the consequences of such process in the corresponding cometary belt. We study the link between the bombardment of massive bodies and mass depletion and eccentricity excitation.


Author(s):  
R.A. Ploc

Samples of low-nickel Zircaloy-2 (material MLI-788-see(1)), when anodically polarized in neutral 5 wt% NaCl solutions, were found to be susceptible to pitting and stress corrosion cracking. The SEM revealed that pitting of stressed samples was occurring below a 2000Å thick surface film which behaved differently from normal zirconium dioxide in that it did not display interference colours. Since the initial film thickness was approximately 65Å, attempts were made to examine the product film by transmission electron microscopy to deduce composition and how the corrosion environment could penetrate the continuous layer.


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