scholarly journals EPR investigation of electronic excitations in rare gas solids (Review Article)

1998 ◽  
Vol 24 (10) ◽  
pp. 693-707 ◽  
Author(s):  
R. A. Zhitnikov ◽  
Yu. A. Dmitriev
ChemInform ◽  
2010 ◽  
Vol 30 (43) ◽  
pp. no-no
Author(s):  
R. A. Zhitnikov ◽  
Yu. A. Dmitriev

2000 ◽  
Vol 12 (12) ◽  
pp. 2769-2781 ◽  
Author(s):  
A N Ogurtsov ◽  
A M Ratner ◽  
E V Savchenko ◽  
V Kisand ◽  
S Vielhauer

2001 ◽  
Vol 15 (28n30) ◽  
pp. 3685-3689
Author(s):  
IGOR GOLINEY ◽  
VOLODYMYR SUGAKOV

Energy spectra of the size quantization of excitons in Xe, Kr, Ar and Ne precipitates in Al and their manifestation in reflection spectra are calculated taking into account polariton effects (dipole-dipole exciton interactions), spatial dispersion and mixing of the electronic excitations of the inclusion with collective excitations of the surrounding metal (plasmons). It was shown that: 1) the proximity of energies of the exciton levels and the plasmons localized on the inclusion (surface plasmons) results in the gigantic shift (up to 1 eV) of the levels of coupled excitations, 2) the transfer of the oscillator strength from the plasmon level to the exciton levels leads to the amplification of optical transitions in bubbles by several orders of magnitude. Depending on the position of the surface polariton with respect to the surface plasmon the spectra either show additional broadenning due to the coupling with quantized exciton levels (Ar, Ne) or the polariton level is pushed out of the exciton band and manifests itself as a narrow dip in the reflection spectra.


2007 ◽  
Vol 76 (10) ◽  
Author(s):  
Wolfgang Harbich ◽  
Christoph Sieber ◽  
Karl-Heinz Meiwes-Broer ◽  
Christian Félix

1966 ◽  
Vol 24 ◽  
pp. 348-349
Author(s):  
Th. Schmidt-Kaler

This is only an informal remark about some difficulties I am worrying about.I have tried to recalibrate the MK system in terms of intrinsic colour (B–V)0and absolute magnitudeMv. The procedures used have been described in a review article by Voigt (Mitt. Astr. Ges.1963, p. 25–35), and the results for stars of the luminosity classes Ia-O,I and II have been given also in Blaauw's article on the calibration of luminosity criteria in vol. III (Basic Astronomical Data, p. 401) ofStars and Stellar Systems.


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