Spectral Diffusion in Organic Glasses:  Time Dependence of Spectral Holes

1996 ◽  
Vol 100 (51) ◽  
pp. 19945-19953 ◽  
Author(s):  
J. M. A. Koedijk ◽  
R. Wannemacher ◽  
R. J. Silbey ◽  
S. Völker
Keyword(s):  
Time Dependence ◽  
Spectral Diffusion ◽  
Organic Glasses

Spectral diffusion induced by energy transfer in doped organic glasses: Delay-time dependence of spectral holes

1999 ◽  
Vol 110 (2) ◽  
pp. 1010-1016 ◽  
Author(s):  
F. T. H. den Hartog ◽  
C. van Papendrecht ◽  
R. J. Silbey ◽  
S. Völker
Keyword(s):  
Energy Transfer ◽  
Time Dependence ◽  
Delay Time ◽  
Spectral Diffusion ◽  
Organic Glasses

Ground state tunneling and optical spectral diffusion in organic glasses

1984 ◽  
Vol 80 (7) ◽  
pp. 3496-3497 ◽  
Author(s):  
W. Breinl ◽  
J. Friedrich ◽  
D. Haarer
Keyword(s):  
Ground State ◽  
Spectral Diffusion ◽  
Organic Glasses

Nonequilibrium phenomena in spectral diffusion physics of organic glasses

1996 ◽  
Vol 105 (5) ◽  
pp. 1798-1806 ◽  
Author(s):  
K. Fritsch ◽  
J. Friedrich ◽  
B. M. Kharlamov
Keyword(s):  
Spectral Diffusion ◽  
Nonequilibrium Phenomena ◽  
Organic Glasses

Spectral diffusion induced by energy transfer and high-pressure effects in doped organic glasses: A hole-burning study

1995 ◽  
Vol 66-67 ◽  
pp. 1-7 ◽  
Author(s):  
F.T.H. den Hartog ◽  
M.P. Bakker ◽  
J.M.A. Koedijk ◽  
T.M.H. Creemers ◽  
S. Völker
Keyword(s):  
High Pressure ◽  
Energy Transfer ◽  
Spectral Diffusion ◽  
Pressure Effects ◽  
Hole Burning ◽  
Organic Glasses ◽  
High Pressure Effects

The O–C diagrams of minor planets − a new approach to modelling the rotation

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss
Keyword(s):  
Error Analysis ◽  
Time Dependence ◽  
Theoretical Work ◽  
Minor Planet ◽  
Minor Planets ◽  
New Approach ◽  
Preliminary Results ◽  
Ccd Observations

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.

Influence of the hyperfine structure on the time-dependence of Mössbauer transmission

1985 ◽  
Vol 46 (8) ◽  
pp. 1387-1393 ◽  
Author(s):  
D.L. Balabanski ◽  
E.I. Vapirev ◽  
P.S. Kamenov
Keyword(s):  
Time Dependence ◽  
Hyperfine Structure
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