It is known that fluorescence of trapped
Yb+ ions fades with continuous driving of the
2 S1/2${\mathrm{\ensuremath{-}}}^{2}$
P1/2 transition in the presence of buffer gases. This phenomenon has been interpreted as being caused by population trapping in the
2 F7/2 state of
Yb+ . As another cause of the fluorescence disappearance, we found the production of
YbH+ by chemical reaction of
Yb+ in excited states with
H2 gas. We found that the wavelengths of 369.482, 369.202, and 368.947 nm, formerly assigned as wavelengths for deexcitation of
Yb+ in the
2 F7/2 state to the
2 S1/2 ground state, are actually photodissociation lines of
YbH+ . The change of the resonance point of rf resonance absorption signals indicates the production and dissociation of
YbH+ ions. The production of
YbH+ may be a problem in establishing frequency standards using buffer-gas-cooled
Yb+ , owing to difficulty in removing
H2 gas from vacuum systems.
The UV absorption spectra of thallium halide vapors consist of a series of peaks corresponding to various photodissociation channels leading to the formation of different states of the product atoms.1 There has been renewed interest in determining the yields of different states of the metal atom produced by photodissociation of the thallium halides, particularly with a view to establishing conditions for selective production of metastable excited states for anti-Stokes Raman shitting2 and other purposes.
Experimental data are presented which demonstrate superfluorescent radiation due to stimulated transitions between the lowest-bound diatomic states of xenon and the repulsive ground state. In this context, superfluorescence describes a condition where, even in the absence of feedback, radiation from the fluorescent medium is dominated by stimulated transitions. The continuum emission spectrum was highly anisotropic and narrowing of the spectrum was observed. The optical gain was greatest at a wavelength of 1730 ± 10 Å, where the experimentally estimated effective gain cross section is 1 × 10−18 cm2.
Bose-Einstein condensation, an effect long known for material particles as cold atomic gases, has in recent years also been observed for photons in microscopic optical cavities. Here, we report absorption and emission spectroscopic measurements on the lowest electronic transition ($5{p}^{6}\ensuremath{\rightarrow}5{p}^{5}6s$) of xenon, motivated by the search for a thermalization medium for photon Bose-Einstein condensation in the vacuum-ultraviolet spectral regime. We have recorded pressure-broadened xenon spectra in the 135- to 190-nm wavelength regime at conditions near the critical point. The explored pressure and temperature ranges include high-pressure gaseous xenon below the critical pressure and supercritical xenon at room temperature as well as liquid xenon close to the boiling point near the critical pressure.