rotational spectroscopy with an optical centrifuge
TRANSCRIPT
This journal is© the Owner Societies 2014 Phys. Chem. Chem. Phys., 2014, 16, 4071--4076 | 4071
Cite this:Phys.Chem.Chem.Phys.,
2014, 16, 4071
Rotational spectroscopy with an opticalcentrifuge
Aleksey Korobenko,*a Alexander A. Milner,a John W. Hepburnb and Valery Milnera
We demonstrate a new spectroscopic method for studying electronic transitions in molecules with extremely
broad range of angular momentum. We employ an optical centrifuge to create narrow rotational wave
packets in the ground electronic state of 16O2. Using the technique of resonance-enhanced multi-photon
ionization, we record the spectrum of multiple ro-vibrational transitions between X3Sg� and C3Pg electronic
manifolds of oxygen. Direct control of rotational excitation, extending to rotational quantum numbers as
high as N \ 120, enables us to interpret the complex structure of rotational spectra of C3Pg beyond
thermally accessible levels.
The dynamics and spectroscopy of highly excited states of molecules
is an issue of great importance to chemical physics. Perturbative
approaches do not always work at high levels of excitation, where
coupling between degrees of freedom changes dramatically from
what is observed at thermal energies.1 As a result, interpreting
molecular spectra becomes increasingly difficult as the level of
excitation grows.2 Significant geometric changes in highly excited
molecules, when the level of excitation exceeds an isomerization
barrier, make understandingmolecular spectroscopy in these energy
ranges an ongoing challenge.4,5
This challenge can become more acute in the case of spectro-
scopic studies of a process, where product molecules can be
formed in highly excited states.6,7 To detect the low density
products, resonance-enhanced multiphoton ionization (REMPI)
is often employed due to its high sensitivity, spectral resolution
and versatility.8,9 This means that the electronic spectroscopy of
a highly rotationally excited molecule must be understood, both
the assignment of resonances and their strengths. This task can
be complicated by a predissociative coupling and decay behavior
in the intermediate excited electronic states.10
Assuming that the molecule of interest is reasonably stable,
REMPI spectra recorded at high temperatures can provide
information on the properties of highly excited states, but this
approach is limited both by the temperatures that themolecule can
tolerate before it dissociates, and by the difficulty of unraveling the
complex spectrum of a high temperaturemolecule, as illustrated by
the work done on the spectrum of high temperature water.2 In the
case of oxygen, reaching the high rotational states probed in
this paper (N > 100) would require a temperature ofE50 000 K.
Rotational excitation of oxygen with strong ultra-short laser
pulses is limited to N B 40 due to the rapidly increased
ionization rate with growing laser intensities.3 Even if a broad
thermal distribution of highly excited rotational states could be
produced in a diatomic molecule such as oxygen, the triplet
structure of the ground and excited states coupled with two-
photon selection rules (for the C3Pg (v0 = 2)’’ X3Sg
� (v00 = 0)
transition), would result in as many as 21 overlapping rotational
branches, making spectroscopic assignment challenging.11
Optical centrifuge is an alternative tool for exciting molecules
to extremely high rotational states by means of non-resonant laser
fields.12–15 In a recent study, we have shown that the centrifuge
can be used to produce and control the so-called ‘‘super rotor’’
states – coherent rotational wave packets with ultra-high angular
momentum N and narrow distribution width dN { N.16 Here we
utilize this unique capability of the centrifuge for the purpose of
obtaining and interpreting complex REMPI spectra of oxygen
super rotors (0o Nt 120). We excite oxygen to a narrow rotational
wave packet whose center is accurately tuned across the broad range
of well defined N values. The centrifuge excitation is then followed
by a REMPI measurement. Owing to the narrow N distribution, the
detected spectrum becomes significantly less congested, and identi-
fying rotational resonances is greatly simplified.
Following the original recipe by Karczmarek et al.,12 we utilize
the output of an 800 nm, 35 fs (full width at half-maximum,
FWHM), Ti:Sapphire regenerative amplifier. We split its spectrum
in half at around the central wavelength (Fig. 1a), in a Fourier
plane of a pulse shaper. Frequency chirps of equal magnitude
(0.26 ps�2) and opposite signs are applied to the ‘‘red’’ and ‘‘blue’’
arms of the centrifuge, as demonstrated by the cross-correlation
frequency-resolved optical gating (XFROG) measurement (Fig. 1c).
The latter was carried out by overlapping the centrifuge pulse
with a reference Fourier-transform limited pulse on a 20 mm-thick
BaB2O4 crystal. The bandwidth of the reference pulse was reduced
aDepartment of Physics & Astronomy, University of British Columbia,
2036 Main Mall, Vancouver, BC, Canada V6T 1Z1. E-mail: [email protected] of Chemistry, University of British Columbia, 2036 Main Mall,
Vancouver, BC, Canada V6T 1Z1
Received 30th October 2013,
Accepted 9th January 2014
DOI: 10.1039/c3cp54598a
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to about 1 nm in a separate pulse shaper to increase the spectral
resolution. The spectrum of the frequency mixing signal was
measured as a function of the relative time delay between the
centrifuge and reference pulses.
The two centrifuge arms are combined with a polarizing
beam splitter cube, and polarized with an opposite sense of
circular polarization. Optical interference of the two circularly
polarized frequency-chirped laser fields results in a pulse with
rotating linear polarization (inset to Fig. 1c). Because of the
anisotropic polarizability, molecular axes line up along the axis
of laser polarization, and then follow it adiabatically as
the plane of polarization rotates with increasing angular
frequency. Quantum-mechanically, this process corresponds to
the rotational ladder climbing, executed as a series of consecutive
Raman transitions between the rotational levels separated by
DN = 2. Each step consists of absorbing a photon from the blue
centrifuge arm and emitting a photon into the red arm. The
frequency difference between the two photons (2O) grows in
time following the rotational line separation. Opposite circular
polarization of the two centrifuge arms ensures DMN = 2
selection rule, resulting in unidirectional rotation. Given the
available spectral bandwidth, the accelerating centrifuge
can reach angular frequencies on the order of 10 THz, which
in the case of oxygen corresponds to the rotational quantum
number N E 119.
As we have demonstrated in ref. 16 truncating the spectrum
of the centrifuge in a Fourier plane of the pulse shaper by a
movable shutter (see inset to Fig. 1a, and field spectrum in
Fig. 1b) enables accurate control of the rotational state of the
centrifuged molecules. Characterizing the centrifuge field with
XFROG allowed us to calibrate the final rotation speed of the
centrifuge, and hence the corresponding molecular angular
momentum, as a function of the shutter position.
REMPI detection was carried out using narrowband nano-
second probe pulses tunable from 279 nm to 288 nm (0.1 cm�1
line width, 500 mJ per pulse, 50 Hz repetition rate). The probe
beam was combined with a centrifuge beam (5 mJ per pulse) on
a dichroic mirror (Fig. 2), and focused with a 35 mm focal length
spherical aluminium mirror on a supersonically expanded mole-
cular jet passing between the charged plates of the time-of-flight
(TOF) mass spectrometer. We estimate the peak centrifuge field
intensity at the focal spot around 1013 W cm�2. The jet was
generated by an Even-Lavie pulsed valve (25 ms opening time,
150 mm nozzle diameter) located 20 cm away from the detection
region. Ion current was detected with a microchannel plate
(MCP) detector. The initial rotational temperature of the sample,
extracted from the REMPI spectrum taken without the centrifuge
field (Fig. 3a), was about 10 K.
The main result of this work is shown in Fig. 3, where
the detected ion count is plotted against the probe energy
(horizontal axis) and the final rotation speed O of the truncated
centrifuge (vertical axis). The latter is expressed in terms of the
angular momentum N of an oxygen molecule rotating with the
angular frequency O, according to:
O = 2pc[E(N) � E(N � 1)],
E(N) = BN(N + 1) � DN2(N + 1)2,
where E is the energy of state |Ni, c is the speed of light in
vacuum, B = 1.438 cm�1 and D = 4.839� 10�6 cm�1.18 The validity
of Dunham expansion of rotational energy to second order in
Fig. 1 Optical centrifuge. (a) Broadband laser pulses from a Ti:S chirped pulse amplifier (10 mJ, 35 fs, 1 KHz repetition rate) are dispersed with a
diffraction grating and split in the center of the spectrum in a Fourier plane of the focusing lens into ‘‘red’’ and ‘‘blue’’ arms, whose chirps are individually
controlled by two separate ‘‘chirp boxes’’. The chirp of the ‘‘red’’ arm is reversed, while that of the ‘‘blue’’ arm is left unchanged. Movable shutter on a
motorized linear stage (inset) allows precise truncation of the ‘‘blue’’ arm bandwidth. (b) Spectrum of the centrifuge pulse after shaping. Solid red (dashed
black) line corresponds to the truncated (full) centrifuge. (c) Cross-correlation frequency-resolved optical gating (XFROG) spectrogram of the truncated
centrifuge field, schematically shown below the XFROG plot. O is the angular frequency at which molecules are released from the centrifuge.
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N(N + 1) at extremely high values of N has been demonstrated
in our previous study.16
Each peak in the two-dimensional REMPI spectrogram of Fig. 3b
corresponds to a two-photon transition between a rotational
level in the electronic ground state, X3Sg�, and a rotational level
of C3Pg. The finite horizontal width of the observed peaks
stems from the predissociation line width (as in conventional
‘‘1D REMPI’’ detection), whereas finite vertical spread reflects
the narrow width of the excited rotational wave packet created
by the centrifuge.
The complexity of the two-photon absorption line structure
in rotationally hot oxygen gas is illustrated by red and yellow
lines in Fig. 3a which correspond to the hot thermal ensemble
(simulated numerically) and the ensemble of centrifuged mole-
cules (experimentally observed 2D spectrogram integrated along
its vertical dimension), respectively. In sharp contrast to conven-
tional 1D REMPI spectroscopy, controlled centrifuge spinning
offers direct assignment of rotational quantum numbers to the
observed REMPI peaks, as well as significantly better peak separa-
tion due to their distribution along the added second dimension.
Vertical traces originating from bright resonance peaks in
Fig. 3b (examples are marked with white arrows) correspond to
molecules which ‘‘leaked out’’ of the weakened centrifuge potential
before reaching the terminal angular frequency of the centrifuge.
After escaping the centrifuge, these molecules continue their free
rotation while the trap is accelerating further. The three bright
vertical stripes reproduce the initial cold beam spectrum (blue line
in Fig. 3a) and correspond to the molecules which were not trapped
by the centrifuge. The width of the final rotational wave packets can
be readily extracted as dN E 7 (FWHM), from the vertical cross
sections, shown in Fig. 3c. Here, we detected rotational states withN
as high as B80. Rotational line broadening above N E 60 can be
attributed to the increasing Rydberg-valence interaction (governed
by the Franck–Condon (FC) overlap with the continuum wavefunc-
tions) similarly to the previously observed rotational broadening in
the lower vibrational states (v0 = 0,1) of the excited potential.11
Fig. 2 Detection setup. Centrifuge beam is combined with a tunable UV
laser pulse and focused inside a vacuum chamber on a supersonically
expanded oxygen jet between the charged plates of a time-of-flight (TOF)
mass spectrometer. The ionization rate is measured with a multi-channel
plate (MCP) detector.
Fig. 3 2D REMPI spectrogram for a linearly polarized probe. (a) Experimental spectra of cold (10 K, blue) and centrifuged molecules (yellow), along with a
simulated spectrum of a ‘‘hot’’ thermal ensemble (3000 K, red) calculated with pgopher software.17 (b) Ion signal as a function of the probe laser two-
photon energy and molecular angular momentum defined by the centrifuge final rotation speed. Different areas of the 2D plot were measured with
different sensitivities and probe intensities and are displayed with different color scales to compensate for the broad dynamic range of the data. (c)
Vertical cross-sections of several consecutive peaks from one particular branch, shown in the inset to b. The peaks are regularly separated with a distance
of DN = 2 reflecting 16O2 nuclear spin statistics.
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One can see that the peaks in Fig. 3 are grouped in regular
patterns, resembling Fortrat parabolas corresponding to different
rotational branches. Within a single branch, the center of each
consecutive resonant peak is shifted by DN = 2 (Fig. 3c), reflecting16O2 nuclear spin statistics. Circularly polarized light can be used
to further simplify the spectrum. As shown in Fig. 4, the signal
strength of different rotational branches depends on the handed-
ness of probe polarization. This is due to the highly non-uniform
population distribution among the magnetic sub-levels in the
centrifuged wave packet, withmost of the population concentrated
at MNC N (or MNC �N).12
To identify different rotational branches, we use three sets of
molecular constants (for F1,F2 and F3 spin–orbit components of
the excited state) from the previous studies on thermally excited
ensembles.7,19 The three components correspond to L + S = 0
(F1), 1 (F2) and 2 (F3), with L and S being the projections of the
orbital and spin components of the total angular momentum
on the molecular axis, respectively. These constants are listed
in Table 1. For F2 and F3 components, our results are well
described by the constants provided by Lewis et al.19 On the
other hand, the observed F1 peaks do not agree well with the
suggested numerical values (n0 = 69366 cm�1 and B0 = 1.6 cm
�1),
as shown in Fig. 5. This can be attributed to the complexity of
the broadened and highly overlapping structure of F1 lines,
which makes it hard to interpret and fit the data from a
thermally populated ensemble. Centrifuge spectroscopy enables
us to correct the values of F1 molecular constants (Table 1)
by performing the fit of the most pronounced DN = �2
branch (Fig. 5).
The lowest vibrational level of C3Pg electronic state of
oxygen known to exhibit well-resolved rotational structure is
v = 2.11 Predissociation to the closely lying valence state 13Pg
broadens the rotational spectrum of the lower vibrational states
v = 0,1. This broadening is weakened in the case of v = 2
because the repulsive potential crosses the level near the node
of the vibrational wavefunction, lowering the Franck–Condon
overlap.11 The FC overlap, however, increases with the increasing
degree of rotational excitation. At high values of N, we observe a
significant line broadening which results in a completely unresol-
vable rotational structure at N\ 60 (see Fig. 3).
At even higher centrifuge frequencies, corresponding to
the extreme rotational levels with 99 o N o 125, we observe
the re-appearance of narrow resonances shown in Fig. 6. Their
line width drops down to a well-resolvedB7 cm�1, as shown in
Fig. 7. Similar non-monotonic N-dependencies were previously
Fig. 4 2D REMPI spectrogram for a circularly polarized probe. Electric field vector is counter-rotating (a) and co-rotating (b) with the centrifuged
molecules. The directionality of laser-induced rotation results in the sensitivity of the measured signal to the handedness of probe polarization. The
results of fitting the data to the theoretical model are shown with colored lines and markers for different branches and resonances, respectively (see text
for details). Branch nomenclature is the same as in ref. 11.
Table 1 Molecular constants used to fit the data in Fig. 4
Spin–orbit branch v0/cm�1 B0/cm
�1 D/cm�1
3P0(F1) 69 375 1.585 2.5 � 10�7
3P1(F2) 69 445 1.648 1.0 � 10�5
3P2(F3) 69 550 1.685 1.3 � 10�5
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observed in OD21 where they were used to analyze the repulsive
state. Indeed, according to the Fermi Golden Rule, the line
width is proportional to the predissociation matrix elements
between the bound and the continuum eigenstates, as well
as the density of states in the continuum. As shown in ref. 21
the behavior of both quantities with N can be calculated
numerically and used for extracting the parameters of the
repulsive state from the experimentally observed dependence
on the rotational quantum number.
Our analysis showed that, unlike the previously discussed
branches of C3Pg (v0 = 2) ’’ X3Sg� (v00 = 0), the observed
ultra-high narrow lines originate from the v0 = 1 state, which
displays no resolvable rotational structure at lower rotational
levels, but re-appears at higher J’s. Well described by Hund’s
Fig. 5 Comparison of the observed REMPI data for the perturbed F1spin–orbit component with the calculations based on molecular constants
from this work (red circles), White et al.7 (blue triangles) and Lewis et al.
19
(purple squares).
Fig. 6 Ultra-high rotational resonances of O2. The two panels correspond to two possible ways of fitting the observed resonant branches (apparent
along white dashed lines) to the calculated Hund’s case (b) structure (labeled with markers). In panel a, the upper branch corresponds to DN =�1, and the
lower one to DN = 3, resulting in Bv = 1.620 cm�1 and Dv = 4.4 � 10�6 cm�1. In panel b, the upper branch overlaps with DN = �2, whereas the lower one
with DN = 2, yielding Bv = 1.664 cm�1 and Dv = 5.7 � 10�6 cm�1.
Fig. 7 Observed linewidths of J0 = N0 � 1 (triangles) and J0 = N 0 (squares)
spin–orbit sublevels of C3Pg (v0 = 1) level as functions of rotational
quantum number N0. Inset demonstrates a fit of experimental data (solid
red) to a sum of lorentzians (dashed black) in order to extract line widths.
Absolute position, absolute area and the widths of two peaks were fitted
for each doublet individually, with the areas ratio fixed to a value extracted
from the best resolved N0 = 115 doublet and with a doublet line separation
equal to a calculated one.
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case (b) at such high degree of rotational excitation, the observed
rotational structure consists of a series of spin–orbit multiplets.
Out of 9 possible DN branches, we have observed only
two (dashed lines in Fig. 6). Given this limited amount of
information, fitting the data by a single set of molecular
constants proved difficult. Our analysis resulted in two possi-
bilities shown in panels a and b of Fig. 6. The retrieved
molecular constants are Bv = 1.620 cm�1 and Dv = 4.4 �
10�6 cm�1 for plot a, and Bv = 1.664 cm�1 and Dv = 5.7 �
10�6 cm�1 for plot b. To choose between the two possibilities,
we note that in Hund’s case (a), an effective rotational constant
B0 for F2 spin–orbit component is equal to the true Bv value.20
This implies that at v = 2, Bv = 1.648 cm�1 (see Table 1). Since we
expect Bv to decrease with v, Fig. 6b should reflect the correct
branch assignment.
In conclusion, we have demonstrated a new spectroscopic
method for studying the rotational structure of electronic
transitions in molecules. The method is based on controlled
molecular spinning with an optical centrifuge. We have applied
this technique to C3Pg’’ X3Sg� (v00 = 0) in O2. By varying the
level of rotational excitation, we have observed rotational line
broadening and narrowing associated with the dependence of
predissociation rates on the molecular angular momentum.
In case of v0 = 2, resolved at lower rotational states (N t 60),
we showed an agreement with previously reported molecular
constants for F2 and F3 spin–orbit components and, owing to
the higher resolution of the implemented method, refined
those for the strongly perturbed F1 component. In case of
v0 = 1, extreme rotational excitation (N \ 100) resulted in the
suppression of predissociation and enabled us to determine
previously unknown rotational constants.
Acknowledgements
This work has been supported by the CFI, BCKDF and NSERC,
and carried out under the auspices of the Center for Research
on Ultra-Cold Systems (CRUCS). We gratefully acknowledge
stimulating discussions with R. Krems, V. Petrovic, M. Shapiro
and E. Grant. We would also like to thank one of the reviewers
of this manuscript for pointing out that the dependence of the
rotational line width on N could be used for mapping out
the repulsive potential responsible for the molecular pre-
dissociation. The analysis presented in Fig. 7 is a result of this
valuable suggestion.
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