Lower limit for disappearance rate of F-centers in irradiated alkali halide compounds

Author(s):  
I. E. Makarov ◽  
T. N. Zhukova ◽  
A. K. Pikaev
1982 ◽  
Vol 37 (6) ◽  
pp. 613-614
Author(s):  
A. A. Berezin

Abstract An alkali halide crystal with a high concentration of F-centers is considered. If some of these F-centers are ionized into anion vacancies (a-centers) released electrons can be trapped by other F-centers to form F′-centers. It is shown that for each original concentration of F-centers there is a certain concentration of F′-centers for which the random potential fluctuations due to negatively charged F′-centers and positively charged a-centers have enough amplitude to create Anderson localization condition in the system of F-, F′- and a-centers.


1984 ◽  
Vol 53 (5) ◽  
pp. 1621-1623 ◽  
Author(s):  
Katsuyuki Inabe ◽  
Shoichi Nakamura ◽  
Nozomu Takeuchi

1975 ◽  
Vol 18 (4) ◽  
pp. 541-542
Author(s):  
Yu. M. Annenkov ◽  
V. F. Pichugin ◽  
T. S. Frangul'yan

1996 ◽  
Vol 65 (8) ◽  
pp. 2564-2570 ◽  
Author(s):  
Katsuyuki Matsunaga ◽  
Nobutaka Narita ◽  
Isao Tanaka ◽  
Hirohiko Adachi

2006 ◽  
Vol 48 (3) ◽  
pp. 453-459
Author(s):  
A. N. Varaksin ◽  
A. B. Sobolev ◽  
V. G. Panov

1967 ◽  
Vol 31 ◽  
pp. 117-119
Author(s):  
F. D. Kahn ◽  
L. Woltjer

The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to maintain the random motions in the interstellar gas is estimated as 1051·4±1ergs.


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