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Submitted on 1 Jan 1983
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Observation of optical pumping effects in collinear atomic beam - laser beam(s) interaction
N. Bendali, H.T. Duong, J.M. Saint Jalm, J.L. Vialie
To cite this version:
N. Bendali, H.T. Duong, J.M. Saint Jalm, J.L. Vialie. Observation of optical pumping effects in collinear atomic beam - laser beam(s) interaction. Journal de Physique, 1983, 44 (9), pp.1019-1023.
�10.1051/jphys:019830044090101900�. �jpa-00209686�
Observation of optical pumping effects in collinear atomic beam - laser beam(s) interaction
N. Bendali, H. T. Duong, J. M. Saint Jalm and J. L. Vialie
Laboratoire Aimé Cotton (*), C.N.R.S. II, Bâtiment 505, 91405 Orsay Cedex, France
(Reçu le 9 mai 1983, accepté le 26 mai 1983)
Résumé. - La sensibilite de la méthode de détection des résonances optiques par observation de la fluorescence émise par un jet rapide
enexcitation colineaire, est limitée par le pompage optique. Dans l’ expérience décrite ici,
nous tirons parti de
cepompage optique en détectant les résonances optiques à l’aide d’un second laser colinéaire,
réalisant ainsi un gain sensible
ensignal de fluorescence. Les effets de la polarisation et de la puissance des faisceaux laser ont été étudiés aussi bien dans le cas de l’excitation d’atomes de Na par un seul laser que par deux lasers.
Abstract.
2014The detection of optical resonances by observation of the fluorescence light emitted from a fast atomic
beam of Na interacting with
acollinear laser beam is limited in sensitivity by optical pumping processes. In the
experiment reported here, we take advantage of the optical pumping by using a second collinear laser beam, achieving then
again in fluorescence signal. The effects of the lasers power and polarization on line shapes have been
studied in the single laser excitation case as well
asin the two laser beams one.
Classification
Physics Abstracts
32.80
1. Introduction.
In recent years, a great deal of experimental effort has
been devoted to systematic studies of hyperfine
structure and isotope shifts of long isotopic sequences
including short lived nuclides far from stability, in large part because of their importance to understanding
nuclear properties [1]. Since most of the on line work
is performed at isotope separator facilities, one has to deal with ion beams. Since resonance lines of ions are
mostly inaccessible to CW single mode dye lasers, the ions have to be converted into neutral atoms. In the method of laser spectroscopy on fast atomic beam [2],
the ion beam is very efficiently converted by charge exchange collisions into atomic beam with unchanged phase space distribution. The narrowing of the velocity spread resulting from the initial ion acceleration is then conserved and consequently the residual Doppler
width may be within the natural linewidth. Therefore,
in collinear excitation, most of the atoms of the beam may be simultaneously resonant with the laser light giving to the method high resolution and high sensi- tivity capabilities. Optical resonances are detected by
observation of the fluorescence light. The highest sensitivity is obtained when the fluorescent photon
yield per atom is not limited by optical pumping
processes. Resonances have been detected with an atomic flux of 1O5/s in the case of the strong resonance line 180-1 P 1 of BaI, for isotopes having no hyperfine
structure [3]. If there is a hyperfine structure in the ground state, the atoms are removed from the absor- bing ground state level within a few, optical pumping cycles, thus limiting the fluorescence yield of the experiment to a few photons per atom. Instead of bearing with it, we proposed to take advantage of the optical pumping to detect optical resonances by
means of a second collinear laser beam acting as a
detector of the pumping process [4]. The experiment reported here is intended to check the gain in sensitivity
obtained with this method when applied to a sodium
atomic beam.
2. Experimental conditions.
Figure 1 presents a schematic diagram of the appa- ratus. The Na+ ions are produced at the oven exit by
ionization of the Na vapour on the inner surface of a
tantalum tube heated by d.c. current up to about 1200 OC [5]. After acceleration up to 5 kV and focusing by an einzel lens, the ion beam is deflected by 100 in an
electrostatic parallel-plate deflector and set collinear with the laser beam. The fast atomic beam is obtained
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:019830044090101900
1020
Fig. 1.
-Experimental set-up.
by charge transfer collisions in a cell of recycled
sodium vapour [6, 7]; the vapour pressure at the centre of the cell is around 10 - 3 torr. The geometrical
factors are the length of charge exchange cell (L1
=26 cm), the length of fluorescence observation zone
(L2
=6 cm), the distance between the centres of these two zones (L3
=35 cm in a first set of experiments and L3
=60 cm afterwards). Intensities of ion and neutral beams are monitored by Faraday cups; their shapes
are controlled by two beam scanners. Beam scanners
are also useful to finely adjust the collinearity of the
fast atomic beam with the laser beam.
The dye lasers are CW ones single mode and tunable
(Coherent Radiation 599 Model). One of these lasers is
frequency piloted by a sigmameter [8]. Frequency
sweep of the other one is done by the standard Cohe- rent Radiation scanning system. With respect to the ion beam, each laser beam can be sent either co- or counter
propagating. Although we have tested Doppler tuning by varying the atomic beam velocity by means of a post acceleration voltage applied to the charge exchange cell, we prefer to scan the laser frequency with the help
of the sigmameter. Moreover in the experiments using two different laser beams (see below) the two
laser frequencies must be independently varied and velocity tuning is therefore unadequate. For each laser
beam a half-wave plate Pl,2 and a Glan-Thomson
prism G1,2 allow us to adjust the polarization direction
and the intensity of the laser light. The two laser beams
are superposed on a dichroic mirror. Atomic fluores-
cence is detected by a cooled photomultiplier. No photon counting technique has been used since the
intensity of the atomic beam is in the range of 101 ° par- ticles/s. The background, resulting essentially from
laser stray light, is reduced by a carefully designed
blackened observation zone.
3. Fluorescence signal observed with one collinear laser beam.
The hyperfine structure (hfs) of the D
1line is well known, it is reproduced in the insert of figure 2.
Figure 2 also shows a scan of the D1 line obtained
with a 100 uW linearly polarized laser beam. On the low frequency side of each peak appears a small satellite resonance, labelled (a). It corresponds to the
Fig. 2.
-Fluorescence signal
as afunction of the frequency,
in the D1 line, observed with
onecollinear laser beam.
inelastic charge transfer via the 3p doublet [9]. The frequency difference between one peak and its satellite
(~ 70 MHz) reflects an energy loss of about 2 eV, corresponding to the 3p-3s energy difference.
The observed relative intensities of the four hyper-
fine components correspond to the theoretical ones.
The linewidth obtainable in collinear laser spectro-
scopy has been discussed in details [10]. In our case we
measured a frequency width (FWHM) of 28 MHz, comparable to the best results reported by Anton
et al. [2] for sodium fast beams. This linewidth is mainly
due to the initial kinetic-energy spread of the ions before acceleration. The energy spread corresponding
to a width of 28 MHz is 0,7 eV; it is larger than the
thermal spread calculable for a temperature of 1 200 OC of the ion source and is probably due to the heating d.c. voltage (~ 2 V) applied to the tantalum tube. One observes, indeed, that the linewidth of the
resonances increases very rapidly with the heating
current intensity. As the light power is increased, the
resonances broaden (see Fig. 3). This broadening is a
consequence of the hyperfine optical pumping pro-
cesses occurring during the atoms flight from the charge-exchange cell to the detection zone; this
pumping transfers the atoms from the resonant hyper-
fine ground level to the non resonant one. Its efficiency
is maximum at exact resonance and decreases with laser detuning; therefore, in the detection zone, the
population of the resonant ground level is minimum at exact resonance. This explains the observed line
broadening. It occurs at low laser power ( 1 mW)
for which the usual power broadening is negligible.
At further increase of the light power each fluorescence line exhibits a dip at exact resonance. For the F
=1 -> F’
=2 transition the dip is easily observable
and the signal falls down to zero with increasing laser
power. For the three other components, F=1
-F’=1 and F = 2 -+ F’= 1, 2, the situation is more complicated
since for each of these resonances atoms in one or two Zeeman sublevels cannot be excited. In order to clearly
observe the dips, one has to perform the experiment in
zero magnetic field, thus avoiding a mixing of Zeeman
Fig. 3.
-Effect of an increasing light intensity
onthe lineshape in the D1 line (cancelled magnetic field).
states induced by the earth magnetic field. The curves
shown on figure 3 are recorded with cancelled magnetic
field. Due to the imperfect cancellation of the field,
at very high laser power, the dips are less pronounced
for these three components than for the F = I-+> F’ = 2
one.
Figure 7B shows a scan of a part of the D2 line (low frequency components) at low laser power (100 uW).
Due to the residual Doppler width (28 MHz) the
structure of the excited state is not completely resolved.
Moreover the presence of the satellite resonances, mentioned above, may blur the structure : in parti- cular, for copropagating beams, the satellite line
corresponding to the largest component F = 2 -+ F’= 3 falls just in between the two components F = 2-+>
F’ =1,2. This difficulty is overcome by using counter propagating beams. The resolved h.f. components are observed with the expected intensities.
As the light power is increased, only the transition
F=2-F’=3, for ’which no h. f. optical pumping
occurs, can be seen. For this transition one observes the effects of power broadening and optical saturation.
For laser power higher than 10 mW the fluorescence does not increase much more, indicating that the power
broadening (i.e. the Rabi frequency) is of the order of the Doppler width.
4. Fluorescence observed with two collinear laser beams.
Two laser beams are now aligned on the fast atomic beam. The first one, linearly polarized and at a
moderate power, is frequency scanned across the D1
line while the frequency v2 of the second laser is locked to the hyperfine transition F
=2 - F’
=3 of the D2
line. The fluorescence induced by this second laser
gives a measurement of the population of the F
=2 hyperfine ground level. When the variable frequency v 1 is tuned to the transitions F
=2 -> F’
=1, 2, hyper-
fine optical pumping along the beam transfers the atoms to the non resonant ground level F
=1 and
the detected fluorescence light decreases. On the other hand, when the variable frequency v, is tuned to the
transitions F
=1
-F’
=1, 2, optical pumping along
the beam increases the population of the F
=2 hyper-
fine ground level and the detected fluorescence increases. Figure 4 shows a spectrum of the D 1 line
obtained by this method. As expected two positive and
two negative peaks are obtained. This method is very similar to the « in flight » saturated absorption spectro- scopy on fast ion beams developed by Beguin-Renier
et al. [11]. The frequency width of the observed reso- nances depends on the power of the two lasers. For moderate powers ( ~ 1 or 2 mW) of both laser beams,
the observed linewidth ( ~ 24 MHz) falls below the Doppler width of the beam. For a broad longitudinal
beam velocity distribution, one expects that the ulti- mate width available with this method would be twice the natural linewidth (2 y = 20 MHz in our case). One
can also notice, in figure 4, that the satellite resonances
do not appear on the spectrum recorded with this me-
thod, since they correspond to slower atoms which are
off-resonance with the fixed laser. The scan in figure 4
1022
is obtained with high power (30 mW) for the fixed laser.
For the negative resonances the system is a three level system with a common level in the ground state (see insert of Fig. 4). Due to the high power of laser 2, the level of the ground state is split into a doublet arising from dynamic Stark effect [12,13]. This doublet
is visible on the recording for each negative peak.
It disappears when the light power of laser 2 decreases below 10 mW. This is consistent with the observations
reported above (fluorescence of the D2 line with one laser). For the positive resonances, one has a four level system without common level (see insert of Fig. 4).
Fig. 4.
-Fluorescence signal
as afunction of the frequency
vl, in the D1 line, observed with two collinear laser beams.
Therefore, no doublet is observed even with 30 mW power for laser 2. Since the laser power density seen by the atoms is not the same everywhere, and also for
reasons due to Zeeman degeneracy [14], it is impossible,
with this set-up, to draw more quantitative conclusions about power effects. As an other consequence of the three level structure of the system with a common level in the ground state, the amplitudes and widths
of the negative peaks depend strongly on the relative
polarizations of the two laser beams. The effect is
Fig. 5.
-Effect of the relative polarizations of the two laser
beams : @ parallel polarizations. (B) orthogonal pola-
rizations.
obvious on figure 5 : one recording is obtained with
parallel polarizations, the other one with orthogonal polarizations, all parameters being unchanged. In the
same way, the frequency of the scanned laser beam can
be tuned across the D2 line. As for the D1 line, positive
and negative peaks are observed, as shown on figure 6. The two lasers are oscillating at moderate
power (- 3 mW). The two hyperfine component
Fig. 6.
-Fluorescence signal
as afunction of the frequency
V,, in the D2 line, observed with two collinear laser beams :
@ orthogonal polarizations. (B) parallel polarizations.
F
=2 -> F’
=1, 2 appear as negative peaks, as expected. When the variable frequency is tuned to
F
=2 -> F’ = 3, the atomic transition is excited
by the two lasers and the fluorescent light increases.
For this component, the signal is comparable (in
width and amplitude) to the one obtained when using only laser 1.
All three hyperfine components are now resolved.
Fig. 7.
-Comparison of the fluorescence intensities, at the
same