Absolute absorption oscillator strength measurements on the (a3Π-X1Σ) Cameron band system of CO

1971 ◽  
Vol 4 (5) ◽  
pp. 681-683 ◽  
Author(s):  
V Hasson ◽  
R W Nicholls
Keyword(s):  
Oscillator Strength ◽  
Band System ◽  
Absorption Oscillator Strength

Solvation effects on molecular pure radiative lifetime and absorption oscillator strength in clusters

1990 ◽  
Vol 93 (1) ◽  
pp. 147-158 ◽  
Author(s):  
Abraham Penner ◽  
Aviv Amirav ◽  
Joshua Jortner ◽  
Abraham Nitzan ◽  
Joel Gersten
Keyword(s):  
Oscillator Strength ◽  
Radiative Lifetime ◽  
Solvation Effects ◽  
Absorption Oscillator Strength

SUSY SUPERPOTENTIALS FOR A CONFINED HULTHÉN POTENTIAL

2004 ◽  
Vol 19 (37) ◽  
pp. 2757-2764 ◽  
Author(s):  
Y. P. VARSHNI
Keyword(s):  
Quantum Mechanics ◽  
Oscillator Strength ◽  
Wave Functions ◽  
Dipole Polarizability ◽  
Hulthén Potential ◽  
Hulthen Potential ◽  
Variational Wave Functions ◽  
Absorption Oscillator Strength ◽  
Variational Wave ◽  
Good Agreement

A system consisting of an ion and an electron interacting through the Hulthén potential confined in an impenetrable spherical box, with the ion at the centre is considered. Superpotential which is the crucial quantity in supersymmetric quantum mechanics is proposed for the 1s and 2p states. Variational wave functions are thence derived. Energies are calculated from these for different values of the radius of box (R) and these are compared to the exact values; good agreement is shown to exist between the two. The variational wave functions are further employed to calculate the absorption oscillator strength for the 1s→2p transition and the dipole polarizability for different values of R.

scholarly journals The influence of hyperfine structure on some manganese line profiles in the solar spectrum

2003 ◽  
pp. 35-41 ◽  
Author(s):  
Nikola Vitas ◽  
Istvan Vince
Keyword(s):  
Hyperfine Structure ◽  
Oscillator Strength ◽  
Solar Spectrum ◽  
Oscillator Strengths ◽  
Total Absorption ◽  
Line Profiles ◽  
Absorption Oscillator Strength

Taking into account effects of hyperfine structure, we calculated the synthetic solar spectrum for wavelength intervals around nine neutral manganese lines. To estimate values of hyperfine components we used the Oxford total absorption oscillator strength measurements (Booth et al. 1983). We compared observed profiles (Photometric Atlas of the Solar Spectrum from 3000 to 10000 ?(Delbouille et al. 1973)) of selected manganese lines with synthesized profiles in two cases: when hyperfine structure is not and when it is taken into account. By comparing the calculated with observed spectrum, we corrected the total oscillator strengths of all nine selected manganese lines.

Oscillator strengths in the 2 ∑ + — 2 Π band system of OH by the hook method

1967 ◽  
Vol 301 (1466) ◽  
pp. 343-353 ◽  
Keyword(s):  
Oscillator Strength ◽  
Band System ◽  
Oscillator Strengths ◽  
The Absolute ◽  
Vibration Rotation

The hook method has been used to obtain oscillator strengths for twenty lines in three branches of the (0, 0) band of the 2 ∑ + - 2 Π system of OH. It is found that vibration-rotation interaction decreases the effective f -value for this band by about 7% over the first ten lines of each branch. The absolute f -value obtained for the rotationless molecule is f 00 = (14·8 ± 1·3) x 10 -4 . Although this falls within the range of previous measurements, it is nearly twice as large as the value hitherto considered most probable. For the (1, 0) band, in which vibration-rotation inter­action could not be measured, the absolute oscillator strength is found to be (8·9 ± 1·7) x 10 -4 , giving for the relative oscillator strengths the ratio f 10 / f 00 = 0·60 ± 0·10.

Oscillator Strength Measurements in the Vacuum-Ultraviolet by the Emission Method

1988 ◽  
Vol 102 ◽  
pp. 353-356
Author(s):  
C. Goldbach ◽  
G. Nollez
Keyword(s):  
Oscillator Strength ◽  
Vacuum Ultraviolet ◽  
Oscillator Strengths ◽  
Emission Method ◽  
Absolute Scale ◽  
Good Agreement

AbstractThe principles and the realization of an experiment devoted to oscillator strength measurements in the vacuum-ultraviolet by the emission method are briefly presented. The results obtained for the strong multiplets of neutral nitrogen and carbon in the 1200-2000 Å range yield an absolute scale of oscillator strengths in good agreement with the most recent calculations.

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