6533b830fe1ef96bd1297d3b
RESEARCH PRODUCT
Anomalies in radiation-collisional kinetics of Rydberg atoms induced by the effects of dynamical chaos and the double Stark resonance
N.n. BezuglovA. N. KlyucharevVladimir A. SrećkovićAnatolij A. Mihajlovsubject
PhysicsAtmospheric ScienceAtomic Physics (physics.atom-ph)FOS: Physical sciencesAerospace EngineeringResonanceAstronomy and AstrophysicsPhysics - Atomic Physicssymbols.namesakeGeophysicsAstrophysics - Solar and Stellar AstrophysicsStark effectSpace and Planetary ScienceExcited statePrincipal quantum numberRydberg atomRydberg formulasymbolsGeneral Earth and Planetary SciencesEmission spectrumAtomic physicsSolar and Stellar Astrophysics (astro-ph.SR)Excitationdescription
Radiative and collisional constants of excited atoms contain the matrix elements of the dipole transitions and when they are blocked one can expect occurring a number of interesting phenomena in radiation-collisional kinetics. In recent astrophysical studies of IR emission spectra it was revealed a gap in the radiation emitted by Rydberg atoms ($RA$) with values of the principal quantum number of $n\approx10$. Under the presence of external electric fields a rearrangement of $RA$ emission spectra is possible to associate with manifestations of the Stark effect. The threshold for electric field ionization of $RA$ is $E\approx3\cdot10^{4}$ V/cm for states with $n>10$. This means that the emission of $RA$ with $n\ge10$ is effectively blocked for such fields. In the region of lower electric field intensities the double Stark resonance (or F\"{o}rster resonance) becomes a key player. On this basis it is established the fact that the static magnetic or electric fields may strongly affect the radiative constants of optical transitions in the vicinity of the F\"{o}ster resonance resulting, for instance, in an order of magnitude reduction of the intensity in some lines. Then, it is shown in this work that in the atmospheres of celestial objects lifetimes of comparatively long-lived $RA$ states and intensities of corresponding radiative transitions can be associated with the effects of dynamic chaos via collisional ionization. The F\"{o}ster resonance allows us to manipulate the random walk of the Rydberg electron ($RE$) in the manifold of quantum levels and hence change the excitation energies of $RA$, which lead to anomalies in the IR spectra.
year | journal | country | edition | language |
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2013-11-05 | Advances in Space Research |