Populations of Rydberg States of Atoms in Interstellar Medium

Details Populations of Rydberg States of Atoms in Interstellar Medium Populations of Rydberg States of Atoms in Interstellar Medium

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987atsir1516....3g&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1516/JUL, P. 3, 1987

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Interactions of Rydberg atoms with plasma particles lead to lowering of the ionization potential and nonrealization of upper states of atoms. It may be interpreted in terms of decrease of the upper level populations: bn→0. The differential equation for bn with this boundary condition (instead of bn→1) has been solved. The descending branch of the bn-curve has been solved. The descending branch of the bn-curve has been calculated. The result influences the interpretation of observations of carbon recombination lines at decametric waves.

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