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Astron. Astrophys. 358, 276-286 (2000) 3. Deexcitation of Rydberg MatterThe electrons which are excited into the partly delocalized orbitals in RM also give the bonding between the atoms in RM, as in an ordinary metal. The various energy levels for the core level electrons close to the core ions, the RM electrons in the conduction band between the atoms, and the empty intermediate electronic states around the core ions are shown in Fig. 2. The conduction band is approximately half-filled, and the energy required to move an electron from the highest occupied orbital in the conduction band (at the Fermi level) to infinite distance is the surface work function. This energy is small, of the order of a few K at excitation levels of n = 80.
A direct deexcitation process with emission of a photon corresponding to the energy difference
between a level in the RM continuum and a rather low Rydberg state in
the atom or molecule M is not very likely due to the very small
overlap between these states. However, if electrons are released in
the RM by for example energetic particles, or a free electron current
passes through the RM due to external accelerating fields, a direct
capture of this type may take place. The final state is indicated as
nR, which means a Rydberg electron with principal quantum
number n and maximum angular momentum quantum number l.
There is no selection rule for the n value, but a selection
rule for the angular momentum quantum number l must exist, with
the change Two-electron processes are observed in laser Raman spectroscopic experiments in RM (Svensson & Holmlid 1999). This means that when one electron falls down from the RM states, a Rydberg electron in the same atom is excited slightly with a simultaneous large change in the value of l. The complete process may then be written where The RM surviving for a long time at high n values in the range n = 50 - 90 and large binding distances, 0.4-1.2 µm, may finally deexcite by sequential emission of many IR quanta to lower RM states to which the overlap has increased above some minimum value. This means, that the IR transitions to the low n values may take place from upper states with a lower state of excitation than for radiative transitions to not so low n values. ![]() ![]() ![]() ![]() © European Southern Observatory (ESO) 2000 Online publication: June 26, 2000 ![]() |