Atomic Physics Division
Division Overview |
Program Directions |
Major Technical Highlights
Major Technical Highlights
- Radiometry of Hg/Ar Discharges for Lighting Applications. Lighting
accounts for about 40% of all electrical power consumed in the commercial
sector. About 60% of this power is used in fluorescent lamps; thus even small
improvements in these lamps have large potential for energy and cost savings.
Newly evolving fluorescent lamp designs operate with Hg/Ar discharges at higher
current densities and lower Ar pressures than conventional lamps. As part of a
lighting research consortium organized by the Electric Power Research Institute
(EPRI), we have made systematic studies of the radiant output of such
discharges for all significant lines of neutral mercury in the ultraviolet and
visible regions of the spectrum. For this task we constructed a special lamp
that permits variation of the discharge parameters over a wide range of
operating conditions. Of particular importance is the output at 254 nm,
which is efficiently converted to visible light by the lamp phosphor, and the
output at 185 nm, which is less efficiently converted and damages the
phosphor, shortening its life. Our studies have revealed large variations in
the relative strength of these lines with changes in current density and Hg
pressure (see fig. 1).
These results have major implications for improving the efficiency of
fluorescent lamps. Our data are now being used for detailed comparisons with
predictions of computer lamp models by collaborating scientists at
U. Wisconsin and Osram/ Sylvania. (C.J. Sansonetti, J. Curry,
and J. Reader)
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Dependence of
Radiances on Hg Vapor Pressure at Ar Pressure 66 Pa - 5 mm Lamp
Figure 1. Relative radiances of the 185 nm and 254 nm lines of
neutral Hg in discharges at low Ar buffer gas pressure show large variations
with lamp current and Hg vapor pressure as determined by the 20°C, 40°C, or
60°C temperature of the Hg cold spot. |
- Spectral Data for Fusion Research. To provide data for spectra of
moderately charged ions of interest for the diagnostics of edge regions of
tokamak plasmas, we have carried out a new analysis of the spectrum of
three-times-ionized niobium, Nb3+. Niobium is a highly refractory
material that may play a role in the design of armor plates for future tokamaks.
For this analysis high-resolution spectra of Nb in the 30 nm to
400 nm region were observed with our 10 m vacuum spectrographs. The
analysis was performed with the aid of atomic structure codes that calculate
the expected energy levels and relative intensities in this region. All missing
levels of the lower configurations were located and other configurations newly
determined. By using our high-resolution Fourier transform spectrometer (FTS),
we have also carried out high-precision measurements of spectra of the rare
gases neon, krypton, and xenon in the infrared. These gases are used to blanket
the tokamak divertor regions in order to reduce the heat load on the first
walls. Previously, only calculated wavelengths were available for these spectra.
The observations resolve many questions in the existing descriptions of these
spectra and will be of great use for the diagnostics of a wide variety of
plasmas. (J. Reader, E.B. Saloman, and C.J. Sansonetti)
- High Resolution Spectroscopy for Space Astronomy. Precise atomic
spectral data are needed to interpret stellar spectra from high-resolution
spectrometers on the Hubble Space Telescope. To address this need, we have made
high-precision measurements of wavelengths and hyperfine structure parameters
for a large number of lines of holmium and for selected lines of lead and
bismuth. Determination of the abundances of heavy elements in
chemically-peculiar stars depends critically on the availability and accuracy
of these laboratory data. Our high-resolution FTS was used to measure wave
numbers and hyperfine structure (hfs) constants for approximately 1800 lines of
Ho I and Ho II between 300 nm and 1200 nm. HFS constants
were determined for 300 levels of Ho I and 90 levels of Ho II. The
spectra of Bi I, Bi II and Bi III, which lie at wavelengths too
short for the FTS, were measured with our 10 m normal-incidence vacuum
spectrograph. The wavelength of a 207Pb IV line at 130 nm
was also measured with this spectrograph. As the hfs of this line was too small
to be resolved in the observed spectrum, we devised a scheme to obtain an
accurate estimate of it from the hfs of an analogous line in
199Hg II, which had been measured by the NIST ion storage group
in Boulder. The lead and bismuth results have been used to determine the
abundances of these elements in the stars chi Lupi, HR 7775 and
AV 304. (G. Nave, J. Reader, and C.J. Sansonetti)
- Critical Compilations of Atomic Spectra. We completed work on the
Handbook of Basic Atomic Spectroscopic Data, which provides important energy
level information as well as wavelengths and transition probabilities for
neutral and singly ionized atoms of 99 elements. This handbook will be
published in three types of media: in an electronic book (eBook) format, as a
database on the Web, and as a printed publication. It will form a convenient
resource for spectrochemical and other industrial applications. Also completed
was a new Web database of spectral data needed for the interpretation of
observations from the Chandra X-Ray Observatory. This provides critically
compiled atomic transition probabilities for spectra of Ne, Mg, Si, and S in
the 10 Å to 170 Å region. A compilation containing
critically evaluated transition probabilities for neutral and singly ionized Ba
was completed and a critical review of recent experimental data on Stark widths
and shifts of neutral atoms and positive ions was prepared. (J. Fuhr,
A. Robey, W.C. Martin, L. Podobedova, J. Sansonetti, and
W.L. Wiese).
- Electron-Impact Excitation and Ionization Cross Sections. Cross
sections for excitation and ionization of atoms and molecules by electron
impact are used for the modeling of plasma processing of semiconductors and
plasmas in fusion devices. For atoms such as aluminum, excitation of
inner-shell electrons to the valence shell leads to additional ionization,
because the excited atom has an energy that is higher than the ionization
energy (autoionization). It is difficult to treat this "indirect"
ionization channel using conventional methods such as close-coupling or
R-matrix theory. We have developed new scaling methods that provide simple, yet
reliable ways to calculate cross sections for this type of indirect ionization.
For example, we find that indirect ionization in the Group IIIB atoms (B, Al,
Ga, In, Tl) doubles the total ionization cross section. In the case of Al, by
combining the recently developed binary-encounter-Bethe (BEB) theory for direct
ionization with new scaling methods for indirect ionization, we were able to
explain a factor-of-two discrepancy between experiment and earlier theory,
which did not take account of indirect ionization. For Ga, our new theory
enabled us to choose a preferred data set between two competing sets of
experimental data. The good agreement with the preferred set is shown in
fig. 2. (Y.-K. Kim, M.A. Ali, and P.M. Stone)
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Figure 2. Comparison of theoretical and experimental data for the total
ionization cross sections of gallium. The solid curve labeled "Total"
represents our theoretical calculation that includes indirect ionization. It is
in excellent agreement with the experiment by Patton et al., while theoretical
results that do not include indirect ionization, labeled "Direct" and
"Lotz," reach only about one-half of the peak value obtained from
experiment. |
- Quantum Logic Gates. The ability to coherently manipulate quantum
systems should lead to dramatic breakthroughs in quantum information processing,
quantum communication, and precision measurements. The Quantum Processes Group
has therefore carried out theoretical simulations to show how collisions of
trapped neutral atoms in optical lattice cells may be used to create
entanglement between the atoms, thereby allowing high fidelity quantum logic
gate operations.
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Performing entangling operations requires individual atom control, which might
be achieved by loading atoms into optical lattices. The trap can localize
individual atoms in unique sites to a few tens of nanometers in size, and
provides control over the two-atom entangling operations. Individual trapped
atoms can act as quantum bits, or qubits, by taking advantage of their internal
structure - hyperfine states or long-lived resonant states - or by using the
motional states that result from trapping the atoms.
Our work has characterized the robustness and speed of the entanglement process
when motional states of atoms in a two-color optical lattice form the qubits
and the atom-atom interaction is turned on and off by controling the two laser
intensities. When the barrier separating the individual optical wells is
lowered by changing the relative intensity of the two lasers, the atoms tunnel
through the barrier and the atom-atom interaction entangles the qubits.
Figure 3 illustrates an example of a two-atom wavefunction for the two cases
when the barrier is either high or low. We have shown that by properly
controlling the time-dependent laser intensities a controlled quantum
interference can be used to reduce the decoherence of the entanglement process
to below 0.001% and simultaneously keep the time to entangle the atoms
relatively short. Without the use of the controlled quantum interference a ten
times longer entangling time is needed for the same decoherence rate. Moreover,
we have demonstrated that the idea of using a controlled interference is not
limited to entangling operations of qubits based on neutral atoms. It should be
useful for other qubit implementations as well. (E. Tiesinga,
C.J. Williams, F. Mies, E. Charron)
|
Figure 3. Contour plot of a wavefunction for two interacting atoms in a
one-dimensional double well potential with a barrier between the two wells. A
high barrier localizes one atom in each well, whereas a low barrier allows both
atoms to occupy the same well. |
- Quantum Dot Clusters. The analogy of quantum dots (QD) and
nanocrystals as artificial atoms is now well established and has driven diverse
applications from integrated laser devices to biosensors and biomarkers to
quantum computing. We have explored the next step, the development of
nanocircuits of quantum dot nanodevices, by simulating the properties of
clusters of QDs (artificial molecules and nanoarchitectures) and arrays of QDs
(quantum dot solids).
We developed previously an atomistic tight-binding simulator for the electronic
and optical properties of individual QDs and nanocrystals. This past year we
have extended these simulations to consider artificial molecules, quantum dot
solids and nanoarchitectures. The first step was to understand simple coupled
QDs, as shown in fig. 4 for two core/shell CdS/ZnS nanocrystals, and to
establish the bounds for the analogy between coupled dots and artificial
molecules. Coupled core/shell nanocrystals and stacked pyramidal dots grown by
self-organized molecular beam epitaxy have been simulated. In each case, we
have found that the conduction states in the coupled nanostructures closely
follow the analogy with molecular states. Hybridized conduction states form
and interdot bonds. State energies and polarization depend on this
bonding. Valence-state interdot-hybridization produces significant level
reordering and drastic changes in oscillator strengths. Hybridization of
valence states is complex and cannot be described just in analogy with
molecular hybridization. (G.W. Bryant, W. Jaskolski) |
Figure 4. Schematic diagram of two interacting quantum dots with an
inner core of ZnS and an outer layer of CdS. A typical dot diameter is on the
order of 5 nm. |
- Cold Cesium Mysteries Solved. Researchers in the Quantum Processes
Group have solved a long-standing problem by constructing a quantitative model
of collisions of ultracold cesium atoms. Atomic cesium is an important species
that has been the object of numerous cooling and trapping experiments. Laser
cooled cesium is also the basis of the new NIST F1 cesium atomic fountain clock.
In spite of many studies, a quantitative understanding of collisions of cold
cesium atoms has proved elusive. It is important to understand these collisions,
since collisional shifts in the cesium transition frequency can adversely
affect the performance of the fountain clock. In addition, the collisional
properties of cesium atoms have prevented the achievement of Bose-Einstein
condensation in cold cesium atomic gases.
Collisions of very cold atoms are different from normal high temperature
collisions in that they are strongly affected by special quantum effects
associated with the very long De Broglie wavelength of the colliding
atoms. However, a collision model with only four key parameters characterizes
the full quantum dynamics of cold cesium collisions. Two of these parameters
are known as scattering lengths, which determine clock shifts and the stability
of a Bose-Einstein condensate. One is the coefficient that gives the magnitude
of the long-range force between the two atoms. The other expresses the
effective interaction between the two electron spins as modified by chemical
bonding effects in the cesium dimer molecule. This latter parameter strongly
affects the collisional losses that hinder Bose-Einstein condensation.
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The NIST group set out to explain all previously existing data on cold cesium
collisions. A key to the analysis were new data provided by experiments in the
group of Stephen Chu at Stanford University, which used a magnetic field to
tune a number of cesium dimer bound states to be in resonance with the
colliding atoms. Fitting to the Stanford data determined the four parameters.
The resulting quantitative model not only accounts for all known data on ground
state cold cesium atom collisions but also accurately predicted locations for a
number of resonances prior to measurement.
Figure 5 compares our model calculations (dashed) with typical Stanford
data (solid) on collision rate versus magnetic field. The new model, contrary
to previous expectations, predicts that the collisional shift in a cesium
fountain clock could be greatly reduced if the clock could be operated at a
much lower temperature in the range of 50 nanokelvin. The model also makes
specific predictions for what range of magnetic fields Bose-Einstein
condensation of cesium might be possible. (C.J. Williams,
P.S. Julienne, and P. Leo) |
Figure 5. Inelastic collision rate constant versus magnetic field
(in mT) for two cold, trapped Cs atoms in a particular ground state Zeeman
sublevel. |
- Nano-optics. Nano-optics is a rapidly emerging branch of optics
driven by the need to control and manipulate light on the nanoscale for use in,
for example, photonic devices and circuits, microscopy with nanometer
resolution, and atom trapping and guiding. To fully understand the physics
issues, we have simulated light fields on the nanoscale with applications to
near-field scanning optical microscopy (NSOM), quantum computing and single
molecule spectroscopy.
NSOM has been used intensively at NIST to obtain nanoscale resolution in
optical microscopy. The key to NSOM is to place a nanoscale optical probe in
the near-field of the sample. A critical challenge for NSOM metrology is to
identify and quantify the mechanisms that provide contrast in NSOM images. Even
the simplest samples can provide counterintuitive images that are difficult to
interpret. Holes in a dielectric film appear dark in NSOM images despite the
expectation that probe light would pass most easily through the holes. We have
therefore simulated this case and could show that the image contrast is
determined by how light is extracted from the NSOM probe rather than how the
probe light propagates through the hole. The holes are dark in NSOM images
because less light is extracted from the probe when the probe is above a hole.
This simple but surprising explanation provides another step toward making NSOM
a qualitatively and quantitatively accurate nanoscale metrology.
(G.W. Bryant, A. Rahmani)
- EBIT Tests Remote Temperature Diagnostic. In order to assist NASA
scientists in measuring the temperature of hot plasmas, a team of scientists
from NIST, the Harvard-Smithsonian Center for Astrophysics, the Naval Research
Laboratory, the Observatory of Palermo (Italy), NASA Goddard Space Flight
Center, MIT, and the Lawrence Berkeley National Laboratory have worked together
on an experiment that took place at the NIST EBIT facility. Precisely
controlled x-ray spectra from highly ionized iron and krypton atoms (16 and
26 electrons/atom removed, respectively) were produced by using an intense,
monoenergetic electron beam threaded through a cryogenic ion trap. The highly
ionized atoms were held at a temperature of approximately 5 million Kelvin
while x-rays were measured with a prototype microcalorimeter detector of the
sort being developed for future space missions. Spectra were collected with
better than 6 eV resolution using a single detector that covered the broad
spectral range from 10,000 eV to 500 eV. By simultaneously observing
resonance lines and radiative recombination from the monoenergetic electron
beam, it was possible to determine cross sections for electron impact
excitation of the individual resonance lines. In field observations, the
temperature is inferred from the ratio of spectral line strengths, assuming
that the underlying atomic physics is calculable. But the benchmark spectra and
cross sections obtained from the experiment at the NIST facility indicate that
a key astrophysical temperature diagnostic is not valid. The experiment has
thus stimulated work at other institutions to develop an improved diagnostic.
(E. Takacs, I. Kink, and J.D. Gillaspy)
- Sub-millimeter Wave Spectroscopy of Etching Plasmas. Sub-millimeter
wave absorption spectroscopy has been applied to etching type plasmas for the
identification and monitoring of plasma species. As semiconductor wafer-size
grows and feature-size shrinks, monitoring and control of the basic plasma
chemistry has become increasingly important for ensuring fidelity and
performance of microelectronic devices. Sub-mm wave spectroscopy can monitor
the crucial chemical species and provide the necessary feedback for
understanding plasma processing. Our measurements have concentrated on the use
of a backward wave oscillator (BWO) as the sub-mm wave source since this device
is relatively compact and could easily be utilized in an industrial setting. We
have identified chemical species found in fluorocarbon etching-type plasmas
created in the inductively coupled version of the GEC RF Reference Cell. The
GEC Cell creates plasmas similar to those used in commercial etching reactors,
but has numerous ports for diagnostic access. Spectra from 10 molecules
have been identified including feed gases (CHF3, CF3I),
etching radicals (CF2, CF), etching byproducts (CO, COF2,
SiO, SiF2, SiF) and contaminants (H2O). The diagnostic
has been used to measure the dissociation of CHF3 and the relative
dependence of various species on plasma conditions. Spectral resolution of the
BWO is so high that it could also be used to measure the translational gas
through the Doppler broadening of the absorption line shapes. These gas
temperatures are important input parameters to many plasma models since they
are necessary to relate the measured gas pressure to the actual particle
density in the chamber. The gas temperatures measured of several different
plasma species have all been at or only slightly above room temperature (see
fig. 6). (E. Benck with G. Golubyatnikov and G. Fraser,
Div. 844)
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Figure 6. Second harmonic frequency modulated absorption signal of CF in
a CF4 inductively coupled discharge. The smooth curve is a line
shape model fitted to the data corresponding to a gas temperature of
346 °K. |
- UV Intrinsic Birefringence of CaF2 and BaF2.
We made the first measurements of an intrinsic birefringence in the UV
materials CaF2 and BaF2, which are the primary optical
materials considered for 157 nm optical lithography, to be used for
future-generation integrated circuit fabrication. The measured birefringences
are more than ten times the design tolerances for residual birefringence for
157 nm lithography systems, and all such designs will now have to be
substantially modified to account for this effect. This result was
unanticipated by the industry because it was assumed that the cubic symmetry of
these crystals would insure isotropy of the optical properties, which in fact
is only true for long wavelengths. As can be seen in the plot of our
measurements below, the relatively large magnitudes of the intrinsic
birefringences near 157 nm decrease rapidly to unmeasureable values in the
visible, explaining why previous residual birefringence measurements of these
materials in the visible did not reveal the effect. Our measurements were
done in conjunction with theoretical analyses and calculations by
Z. Levine (Electron Optical Physics Division) and E. Shirley (Optical
Technology Division), shown by the curves in fig. 7. We first showed how
the symmetry of this effect can be exploited for compensation by coupling
lenses with differing crystal axis orientations. We also showed that due to the
opposite sign of the effect for CaF2 and BaF2, it can in
principale be eliminated entirely by creating appropriate mixed crystals
Ca1-xBaxF2. All 157 nm
systems are now being designed using at least one of these correction
approaches. (J.H. Burnett)
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Figure 7. Measurements (symbols) and calculations (curves) of intrinsic
birefringence of CaF2 and BaF2 as functions of wavelength
(with standard uncertainties). |
- Ultracold Collisions. Starting with one laser to photoassociate
slowly colliding atoms into bound states of excited diatomic molecules in a
magneto-optical trap, we then used additional lasers to take these molecules
into either doubly-excited states or to bound ground-state molecules. New
spectroscopy of the uppermost bound states of the triplet ground state of
Na2 has been obtained. In addition, the production of stable
ground-state molecules in a number of these states has been demonstrated and
the detection of the molecules, in a state-selective manner, has been
demonstrated as well. Pulsed-laser, pump-probe photoassociation experiments
were carried out that show indications of the dynamics of the
photoassociation-ionization process. Pairs of atoms are excited to
singly-excited states with a first (pump) pulse and then to doubly-excited
states that autoionize with a second (probe) pulse. In order to autoionize
they must survive on the doubly-excited potential into small internuclear
separations. These experiments have demonstrated the importance of the travel
on the strongly attractive singly-excited molecular potentials in the dynamics
of the process. Population excited to these levels at long range is able to
accelerate toward smaller separations, increasing their chance of survival
against spontaneous emission and also bypassing the angular momentum barriers
that exist on the relatively flat ground-state and doubly-excited-state
potentials. (L. deAraujo, S. Gensemer, K. Jones, and
P. Lett)
- Ultracold Plasmas. In an ultracold plasma produced by
photoionization of a laser-cooled gas of metastable xenon we had previously
measured that, at the coldest and densest parameters we could achieve, the
plasma expanded with seemingly more energy than had been put in by the laser
photons. In a search for a reservoir of negative (i.e., binding) energy in the
form of atoms (which would assure energy conservation) we undertook an
experiment that used selective field ionization to measure the formation of
Rydberg atoms. We found that a substantial fraction (up to 30%) of the plasma
recombines into these neutral Rydberg atoms. Summing up the binding energy in
the Rydbergs did seem to account for the excess expansion energy, but these
atoms were formed over a much longer time period than that of the appearance of
the expansion energy. In fact, significant Rydberg formation occurred even
after the plasma density dropped by 4 orders of magnitude. Based on our
findings, the exact mechanism of the recombination is currently under
investigation by several theoretical groups. The leading explanation is a
"freezing out" of electron-ion correlations present in the plasma as
it expands. We have undertaken collaborations with theoretical groups at Los
Alamos National Lab and Auburn Univ. to address this problem. (M. Lim,
J. Roberts, S. Rolston)
- Optical Tweezers. We have observed real-time adhesion between a
monoclonal antibody and its specific antigen in an experiment using optical
tweezers. Both antibody and antigen molecules are immobilized on the surfaces
of (different) polystyrene microspheres, which are trapped by separate optical
tweezers. The monitoring of spontaneous, thermally driven, successive
attachment and detachment events has allowed a direct determination of the
reaction-limited detachment rate for a single bond and also for multiple bonds.
A second experimental direction has been studying the use of liposomes as
bioreactors. For this purpose we have set up a new experiment employing two
optical-tweezer traps and an optical scalpel (a UV laser that can pierce the
wall of a liposome). With this new apparatus, we are able to trap two liposomes
and fuse them together, thus allowing their contents to mix. In a first
experiment, we demonstrated the fusion of a dye-encapsulated liposome with
another liposome and observed, with fluorescence microscopy, the mixing of the
dye. (K. Helmerson, R. Kishore, and S. Kulin)
- Quantum Computing in Optical Lattices. We have achieved
Bose-Einstein condensation (BEC) in rubidium vapor. A new apparatus was
constructed in which rubidium atoms were loaded from a Zeeman-tuned, slowed
atomic beam into a magneto-optical trap (MOT) and then transferred into a
magnetic trap. The atoms were then evaporatively cooled and condensed into the
lowest energy state in the trap. This source of atoms will be used to load 1-D
and 3-D optical lattices for investigation of different quantum logic gate
designs for neutral atom quantum computing. (B. King, S. Peil,
T. Porto, and S. Rolston)
- Optical Interactions in Bose-Einstein Condensates. An experiment to
observe "dynamical tunneling" was performed in collaboration with
researchers from the University of Queensland, Australia. For a wheel spinning
clockwise or counter-clockwise there is energetically no difference between the
two motions, and classically to reverse the sense of rotation requires the
wheel to stop. But quantum mechanics allows the system to "tunnel"
from one state to another even if it is classically forbidden. Tunneling has
been observed since the early days of quantum mechanics, but usually involves
traversing a barrier that, classically, a particle does not have enough energy
to go over. Dynamical tunneling, predicted in the early 80s, is similar, but
some constant of the motion other than energy classically forbids the quantum
mechanically-allowed motion. We observed classically forbidden motion of atoms
transferring between two modes of oscillation in the potential wells formed by
an amplitude-modulated optical standing-wave. Atoms were loaded from a BEC into
the bottom of the optical potentials, and were induced to oscillate back and
forth by a sudden displacement of the standing wave. The number of atoms in
this particular oscillatory motion was observed to decrease with time, as a
group of atoms began to appear oscillating 180o out of phase with
the initial motion. Eventually, almost all of the atoms ended up in the
out-of-phase motion, but then tunneled back to the initial mode of oscillation
(see fig. 8). We observed up to eight coherent transfers of atoms back and
forth between the two stable motions due to dynamical tunneling. No atoms were
observed to exhibit motion intermediate between the two stable oscillatory
motions (for example, corresponding to atoms stopping and reversing direction),
providing further confirmation that the transfer of atoms was due to dynamical
tunneling. (A. Browaeys, H. Haeffner, K. Helmerson,
W. Hensinger, C. McKenzie, W. Phillips, S. Rolston, and
B. Upcroft)
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Figure 8. Dynamical tunneling in the quantum driven pendulum. The figure
shows the momentum distribution of atoms released from an amplitude-modulated
potential for three different times after a BEC was loaded into the potential
(0.25, 2.25, and 5.25 modulation periods (f=250 kHz)). The classical result
from this system would have the momentum distribution remain stationary in this
stroboscopic picture. It is evident that the state of motion of the atoms is in
fact oscillating back and forth, a signature of coherent dynamical tunneling.
The individual peaks are separated in momentum by 2 ħk which
corresponds to a velocity of 6 cm/s for sodium. |
- BEC in 1-D Lattices. We have performed a series of experiments with
a BEC in a 1-D optical lattice. Making use of the small momentum spread of a
BEC and of atom optics techniques, a high level of coherent control over an
artificial solid-state-like system was demonstrated. We were able to
efficiently load the BEC into the lowest lattice band (and other bands) with
different quasi-momentum q by varying the lattice amplitude and lattice
velocity relative to the BEC. By adiabatically increasing the lattice amplitude,
more than 99% of the BEC could be loaded into the lattice ground state. Such
experiments are needed to evaluate the possibility of using neutral atoms in
off-resonant optical lattice potentials for quantum information processing.
Using either phase or amplitude modulation of the optical lattice, we have
coherently transferred population between various lattice band states. For
example, we have used amplitude modulation to transfer atoms from the ground
band to the second excited band for various initial q, allowing a direct
measurement of the curvature of the second excited band.
We have also demonstrated a large-momentum atom beam splitter based on coherent
Bragg diffraction followed by acceleration of the BEC in an accelerating optical
lattice. Bragg diffraction produces atoms in a coherent superposition of 0 and
2 k, where k is the magnitude of
the wavevector of the laser light. The two momentum states could be loaded
predominantly into two bands of the lattice (fig. 9). Acceleration of the
lattice moved atoms in one band with respect to the other, resulting in a large
final momentum (we demonstrated up to 12 k). We have confirmed that the acceleration is coherent by
constructing an atom interferometer based on this novel beam splitter.
(A. Browaeys, H. Haeffner, K. Helmerson, C. McKenzie,
W. Phillips, and S. Rolston)
Figure 9. Time of flight images of the momentum distribution of a BEC
that was suddenly loaded into an optical lattice (depth = 14 recoil energies),
and held for varying lengths of time (time between each image is
0.5 microseconds). When the BEC is suddenly loaded into a lattice, the
wave function is projected into a superposition of various bands. Since each
band has a different energy, the relative phases evolve in time. When the
lattice is switched off, the populations of the bands are projected onto plane
wave states and interferences result in oscillating populations of the various
diffraction orders. The top picture (simple oscillations) shows the case where
quasi-momentum q= 0 states are populated; the bottom picture depicts the
case when q=1 states are populated by switching on a moving lattice.
- Binding Energy Measurements in Light Nuclei. The binding energy of
the neutron in several light nuclei has been measured at the Institut Laue
Langevin (ILL) using the joint NIST/ILL precision gamma-ray spectrometer that
is coupled to the high flux reactor of the ILL. The spectrometer measures the
wavelengths of gamma-ray photons using crystals whose lattice spacings are
precisely known in SI units and an angle scale that is derived from first
principles. Binding energies are obtained by summing the energies (wavelengths)
of all
-rays in a
cascade connecting the capture and the ground states. Binding energy
measurements are important because (1) they provide high-energy (short
wavelength, 0.2 pm) standards
and (2) they check the consistency of precision gamma-ray and atomic mass
measurements.
Binding energy measurements have been made in 29Si, 33S,
and 36Cl species chosen because of their large capture cross
sections. As an example, the reaction n+35Cl 36Cl+ 's leads to the relation
between atomic masses and the neutron binding energy Sn,
m(n) + m(35Cl) =
m(36Cl) + Sn(36Cl).
The binding energies are 8.6 MeV and the available cascades require
the measurement of -rays in the 5 MeV to 6 MeV range. In the course of
these measurements, we have improved our capability to accurately measure small
diffraction angles (< 0.1°) and pioneered the use of thicker
crystals and better collimation to improve signal to background at high
energies. The relative uncertainty of the binding energy measurements is 2 to 4
parts in 10-7 which is comparable to the relative uncertainty of the
best available atomic mass differences. (E. Kessler with S. Dewey,
Div. 846)
- Upgraded Angle Metrology for Absolute Vacuum X-Ray Wavelength
Determination. NIST's Vacuum Double Crystal Spectrometer measures absolute
x-ray wavelengths from 0.6 Å to 12 Å (1 keV to
20 keV). This is tied to the SI via the lattice spacing of the diffraction
crystals. The measurement of absolute wavelengths also requires accurate
measurement of the angle at which the diffraction condition is satisfied. This
year the crystal angle encoder was upgraded to a device that has smaller errors.
Then a new general calibration approach was developed to determine the encoder
error function so that even these small errors can be corrected. A twelve-sided
optical polygon was used with a nulling autocollimator and the requirement of
circle closure (0° = 360°) to first determine the angles between
adjacent polygon faces. Then the polygon was phased with respect to the encoder,
mapping out its 360° error function twelve points at a time. The fitted error
function and its residuals (fit minus measurement) are shown in
fig. 10 (a) and (b), respectively.
Figure 10. (a) The fitted encoder error function and (b) the
residuals (fit minus measurement) for the NIST Vacuum Double Crystal X-Ray
Spectrometer encoder. |
The magnitude of the error corrections is on the order of
0.5 µrad to 1.0 µrad and the residuals are scattered about
zero with a standard error (k=1) of 0.2 µrad (0.00001°). The
angle measurement uncertainty contributes
< 1 × 10-6 to the relative uncertainty of the
wavelength measurements. This improved calibration scheme will be applied to
high precision angle encoders used with other x-ray diffractometers in the
Division. (L. Hudson)
- Laser System for Long-range Fabry-Perot Interferometry. Fabry-Perot
interferometry provides the highest resolution of any technique for measuring
displacements. The standard practice for measuring a displacement consists of
locking a tunable laser to a Fabry-Perot cavity resonance, varying the length
of the cavity, and monitoring the optical frequency of the laser. This approach
has been useful only for measurements of a rather limited range
(
1 micrometer). In order to increase the
measurement range of Fabry-Perot interferometry, we have built a
computer-controlled scanning laser system that probes two adjacent cavity
modes. Displacements up to 50 mm can be measured without sacrificing
resolution. The system incorporates independent acousto-optic control of the
optical frequencies, and employs frequency modulation spectroscopy to provide
error signals in a region in which the laser noise is shot-noise limited. The
light output was coupled into a single-mode fiber, enabling remote
interrogation of a Fabry-Perot cavity in vacuum. The optical frequencies were
measured relative to an iodine-stabilized laser, providing a frequency
reference with a fractional accuracy of 2.5 × 10-11.
This system complements the progress we have made in heterodyne interferometry
and laser stabilization, and should be of particular interest in future
experiments involving thermal expansion of materials and x-ray
interferometry.
The attainable resolution is illustrated in fig. 11, where we studied the
vibration contributed to a Fabry-Perot interferometer by a turbomolecular
vacuum pump at the second harmonic of its rotation frequency. When the pump was
on, a peak appeared whose amplitude corresponds to an rms displacement of less
than 5 fm, - a size typical of nuclear radii. (J. Lawall,
M. Pedulla, and B. Lantz)

Figure 11. Displacement vs frequency plot for our Fabry-Perot system
that illustrates the available high resolution.
Division Overview |
Program Directions |
Major Technical Highlights
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Online: March 2002 |
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