Natural Line Width for Transient Excitations.

1959 ◽  
Vol 129 ◽  
pp. 456 ◽  
Author(s):  
G. Breit ◽  
M. H., Jr. Hull
Keyword(s):  
Line Width ◽  
Natural Line Width

Resonances with sub-natural line width in iodine vapour driven by a polyharmonic laser light field at λ=515 nm

2002 ◽  
Author(s):  
L.F. Vitushkin ◽  
S.V. Lazaryuk ◽  
S.A. Pul'kin ◽  
L. Robertsson ◽  
M.Z. Smirnov ◽  
...  
Keyword(s):  
Line Width ◽  
Light Field ◽  
Laser Light ◽  
Natural Line Width

The natural line width of low field nuclear magnetic resonance spectra

2010 ◽  
Vol 206 (1) ◽  
pp. 168-170 ◽  
Author(s):  
H. Harcken ◽  
R. Ketzler ◽  
M. Albrecht ◽  
M. Burghoff ◽  
S. Hartwig ◽  
...  
Keyword(s):  
Nuclear Magnetic Resonance ◽  
Magnetic Resonance ◽  
Line Width ◽  
Natural Line Width ◽  
Low Field ◽  
Nuclear Magnetic Resonance Spectra ◽  
Magnetic Resonance Spectra ◽  
Nuclear Magnetic

Measurements of the natural line width and energy shift of the K-mesonic 4f → 3d transition in sulphur

1970 ◽  
Vol 32 (5) ◽  
pp. 399-403 ◽  
Author(s):  
G. Backenstoss ◽  
A. Bamberger ◽  
J. Egger ◽  
W.D. Hamilton ◽  
H. Koch ◽  
...  
Keyword(s):  
Line Width ◽  
Energy Shift ◽  
Natural Line Width

Natural line-width effects in gamma- and X-ray emission rate measurements with semiconductor detectors

1981 ◽  
Vol 184 (2-3) ◽  
pp. 497-503 ◽  
Author(s):  
K. Debertin ◽  
W. Pessara
Keyword(s):  
Line Width ◽  
Emission Rate ◽  
Semiconductor Detectors ◽  
X Ray ◽  
Natural Line Width

Strong-field cyclotron scattering. I - Scattering amplitudes and natural line width

1993 ◽  
Vol 412 ◽  
pp. 351 ◽  
Author(s):  
Carlo Graziani
Keyword(s):  
Scattering Amplitudes ◽  
Line Width ◽  
Strong Field ◽  
Natural Line Width

The Mößbauer Effect of the 129 keV Transition in 195Pt

1970 ◽  
Vol 25 (12) ◽  
pp. 1779-1780 ◽  
Author(s):  
B. Wolbeck ◽  
K . Zioutas
Keyword(s):  
Absorption Line ◽  
Line Width ◽  
Mössbauer Effect ◽  
Branching Ratio ◽  
Resonance Absorption ◽  
Mossbauer Effect ◽  
Natural Line Width ◽  
Resonance Absorption Line ◽  
I 31

Abstract The Mößbauer effect of the 129 keV transition in 195Pt has been observed. By use of a Ge(Li) detector any contribution from the strong 99 keV Mößbauer line could be eliminated. The width of the resonance absorption line corresponds to the natural line width. We derived from the magnitude of the observed Mößbauer effect the branching ratio in the decay of the 129 keV level as I (129)/I (31) = ( 5.7 ± 1.6)% .

New possibilities of obtaining spectral holes narrower than natural line width

1998 ◽  
Vol 76-77 ◽  
pp. 130-133 ◽  
Author(s):  
I. Rebane
Keyword(s):  
Line Width ◽  
Natural Line Width

On the natural line width of absorption lines in strong magnetic stellar fields

1994 ◽  
Vol 214 (1-2) ◽  
pp. 103-114
Author(s):  
Javier Bonatti
Keyword(s):  
Line Width ◽  
Absorption Lines ◽  
Natural Line Width
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