THE ROTATIONAL ENERGY LEVELS OF DIATOMIC MOLECULES IN 4Σ ELECTRONIC STATES

1962 ◽  
Vol 40 (5) ◽  
pp. 598-606 ◽  
Author(s):  
Jon T. Hougen
Keyword(s):  
Experimental Data ◽  
Diatomic Molecules ◽  
Energy Levels ◽  
Electronic States ◽  
Rotational Energy

Expressions are derived for the rotational energy levels of diatomic molecules in 4Σ states. These expressions contain two rho-type doubling parameters (γ's), and thus differ from earlier expressions which contain only one such parameter. The new expressions are in better agreement with the experimental data, though some discrepancy still exists.

On the vibration–rotational energy levels of the hydrogen molecular ion HD+

1985 ◽  
Vol 63 (9) ◽  
pp. 1201-1204 ◽  
Author(s):  
L. Wolniewicz ◽  
J. D. Poll
Keyword(s):  
Diatomic Molecules ◽  
Energy Levels ◽  
Rotational Energy ◽  
New Method ◽  
Dissociation Limit ◽  
Radiative Effects ◽  
Vibrational States ◽  
Hydrogen Molecular Ion ◽  
Molecular Ion ◽  
Quantum Numbers

A new method for calculating vibration–rotational energies of diatomic molecules is discussed and applied to the case of HD+. This method is designed to obtain accurate results for all vibrational states including those close to the dissociation limit. Nonadiabatic, relativistic, and radiative effects are taken into account for all the bound vibrational states with rotational quantum numbers J ≤ 5; the estimated accuracy is of the order of 0.001 cm−1.

scholarly journals Electronic Levels Of Cr2+ Ion Doped In II-VI Compounds Of ZnS – Crystal Field Treatment

2012 ◽  
Vol 56 (1) ◽  
pp. 94-99
Author(s):  
Simona Ivaşcu
Keyword(s):  
Experimental Data ◽  
Crystal Field ◽  
Energy Levels ◽  
Electronic States ◽  
Spin Hamiltonian ◽  
Host Matrix ◽  
Absorption And Emission ◽  
Radiative Transitions ◽  
Impurity Ions ◽  
Hamiltonian Parameters

AbstractThe aim of present paper is to report the results on the modeling of the crystal field and spin-Hamiltonian parameters of Cr2+ doped in II-VI host matrix ZnS and simulate the energy levels scheme of such system taken into account the fine interactions entered in the Hamiltonian of the system. All considered types of such interaction are expected to give information on the new peculiarities of the absorption and emission bands, as well as of non-radiative transitions between the electronic states of impurity ions. The obtained results were disscused, compared with similar obtained results in literature and with experimental data.

Possible new interstellar masers

1980 ◽  
Vol 373 (1753) ◽  
pp. 269-284 ◽  
Keyword(s):  
Population Inversion ◽  
Diatomic Molecules ◽  
Energy Levels ◽  
Rotational Energy ◽  
Stimulated Emission

A collisional mechanism for the production of population inversion in the Λ -doublet sub-levels of the lowest rotational energy levels of diatomic molecules is considered. This leads to the conclusion that not only should the known celestial masers, OH and CH, be capable of exhibiting stimulated emission, but also H F + , HC1 + and SH.

Energy Levels and Electromagnetic Transition of 90-94mo Nuclei Using Ibm-1

2020 ◽  
pp. 149-152
Keyword(s):  
Experimental Data ◽  
Transition Probability ◽  
Energy Levels ◽  
Dynamical Symmetry ◽  
Interacting Boson Model ◽  
Excitation Energies ◽  
Electromagnetic Transition ◽  
Boson Model ◽  
Energy States ◽  
Good Agreement

The energy states for the J , b , ɤ bands and electromagnetic transitions B (E2) values for even – even molybdenum 90 – 94 Mo nuclei are calculated in the present work of "the interacting boson model (IBM-1)" . The parameters of the equation of IBM-1 Hamiltonian are determined which yield the best excellent suit the experimental energy states . The positive parity of energy states are obtained by using IBS1. for program for even 90 – 94 Mo isotopes with bosons number 5 , 4 and 5 respectively. The" reduced transition probability B(E2)" of these neuclei are calculated and compared with the experimental data . The ratio of the excitation energies of the 41+ to 21+ states ( R4/2) are also calculated . The calculated and experimental (R4/2) values showed that the 90 – 94 Mo nuclei have the vibrational dynamical symmetry U(5). Good agreement was found from comparison between the calculated energy states and electric quadruple probabilities B(E2) transition of the 90–94Mo isotopes with the experimental data .

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