Isotope Shift in the X-Ray Spectra of Heavy Elements

1955 ◽  
Vol 98 (1) ◽  
pp. 1-5 ◽  
Author(s):  
M. S. Wertheim ◽  
G. Igo
Keyword(s):  
1954 ◽  
Vol 95 (4) ◽  
pp. 1097-1097
Author(s):  
G. Igo ◽  
M. S. Wertheim
Keyword(s):  

Author(s):  
Noriyuki Kuwano ◽  
Masaru Itakura ◽  
Kensuke Oki

Pd-Ce alloys exhibit various anomalies in physical properties due to mixed valences of Ce, and the anomalies are thought to be strongly related with the crystal structures. Since Pd and Ce are both heavy elements, relative magnitudes of (fcc-fpd) are so small compared with <f> that superlattice reflections, even if any, sometimes cannot be detected in conventional x-ray powder patterns, where fee and fpd are atomic scattering factors of Ce and Pd, and <f> the mean value in the crystal. However, superlattices in Pd-Ce alloys can be analyzed by electron microscopy, thanks to the high detectability of electron diffraction. In this work, we investigated modulated superstructures in alloys with 12.5 and 15.0 at.%Ce.Ingots of Pd-Ce alloys were prepared in an arc furnace under atmosphere of ultra high purity argon. The disc specimens cut out from the ingots were heat-treated in vacuum and electrothinned to electron transparency by a jet method.


1972 ◽  
Vol 12 (2) ◽  
pp. 261-270 ◽  
Author(s):  
C. F. Moore ◽  
G. W. Phillips ◽  
R. St-Laurent ◽  
F. Hopkins ◽  
J. White ◽  
...  

2013 ◽  
Vol 87 ◽  
pp. 31-34 ◽  
Author(s):  
M.K. Alqadi ◽  
Y. Alsenjlawi ◽  
F.Y. Alzoubi
Keyword(s):  

2016 ◽  
Vol 65 (2) ◽  
pp. 93-98 ◽  
Author(s):  
Junko HIROKAWA ◽  
Issei MAEDA ◽  
Shunsuke FURUYA ◽  
Yoshinari ABE ◽  
Keiichi OSAKA ◽  
...  

1952 ◽  
Vol 85 (6) ◽  
pp. 1050-1051 ◽  
Author(s):  
P. Brix ◽  
H. Kopfermann

1998 ◽  
Vol 188 ◽  
pp. 61-64
Author(s):  
Trevor J. Ponman ◽  
Alexis Finoguenov

It is clear that there is an important interplay between galaxies and the group environment. At the velocity dispersions (~ 100 km s−1) characteristic of groups, the galaxies interact strongly, leading to triggering of star formation, and galaxy merging. We can expect to see evidence of such processes through differences in the properties of galaxies in groups compared to field galaxies. Conversely, the galaxies affect their environment, as is apparent from the presence of heavy elements in the hot intergalactic medium (IGM) in groups, which emit characteristic X-ray lines.


Nature ◽  
1966 ◽  
Vol 211 (5053) ◽  
pp. 1085-1085 ◽  
Author(s):  
T. GROOT ◽  
P. C. M. N. BRUIJS ◽  
J. H. T. C. VERBEEK

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