Backward fluorescence
from dense cesium vapor induced by Ti:Sa femtosecond laser
Ticijana Ban, Damir Aumiler and Goran Pichler
Institute of Physics, Zagreb, Croatia
At very high cesium densities almost no light can be transmitted. However,
backward fluorescence excited by the laser entering the vapor can be readily
collected and spectrally analyzed. In the past c.w. and nanosecond lasers have
been used for such observations. We were interested in the excitation of the
backward fluorescence by a Ti:Sa femtosecond laser oscillator. The tuning range
was 700-850 nm and the temperature of an all-sapphire cell was in the 400-600
oC range.
The spectrum was resolved between 280 and 1100 nm with numerous well known
spectral features. However, a few new satellite bands especially in the infrared
region revealed that two potential curves of 0g- symmetry made two avoided
crossings. This interpretation of satellite bands in the near infrared spectral
region has interesting connection with cesium ultracold molecule formation
[1].
The rest of the visible spectrum consisted of numerous atomic emission lines
and a few of molecular origin. We were also interested to compare obtained
backward LIF with high pressure pulsed Cs lamp spectrum [2], which may serve
in further development of cesium discharge lamp.
However, when the excitation wavelength approached 750 nm, we observed entirely
different spectrum with irregular oscillations. Since this wavelength also
correlates with the maximum cone angle (see next poster), we believe that it
might be the consequence of self-phase modulation effect.
References:
[1] C. M. Dion, O. Dulieu, D. Comparat, W. de Souza Melo, N. Vanhaecke, P.
Pillet, R. Beuc, S. Miloševic, and G. Pichler, Photoionization and detection
of ultracold Cs2 molecules through diffuse bands, European Physical Journal
D, 18 (2001) 365-370.
[2] G. Pichler, V. Živcec, R. Beuc, Ž. Mrzljak, T. Ban, H. Skenderovic, K.
Günther and J. Liu, UV, visble and IR spectrum of the Cs high pressure
lamp, Physica Scripta, T105 (2003) 98-100.