APS Division of Nuclear Physics Home
Current research topics
ATTA
Magnetic trapping of Ultracold Neutrons
The Gammasphere dectector
Evidence for neutrino oscillations from the LSND
experiment
Exact
calculations of nuclear systems
The Measurement of the Proton's weak magnetism
2002 Nobel Prize in Physics
Sudbury Neutrino Observatory
Charge and Magnetization
Distributions of the Proton
Pentaquark
Spin Structure of the Nucleon
|
ATTA — A New Method of Trace-Isotope Analysis
Argonne National Laboratory
|
Ultrasensitive trace-isotope analysis has been
an important tool in modern science. Two well developed methods,
Low-Level Counting (LLC) and Accelerator Mass Spectrometry (AMS),
have been used for archaeological dating, medical diagnostic procedures,
and for studying the transport processes in the ocean, atmosphere,
and groundwater. They also have applications in physics, such
as studying cosmic rays and detecting solar neutrinos. We have
recently developed a widely applicable method, Atom Trap Trace
Analysis (ATTA) [1], and demonstrated its feasibility by analyzing
two rare isotopes in a natural krypton sample at the parts-per-trillion
level. ATTA can enhance the capability and expand the applications
of ultrasensitive trace-isotope analysis.

Figure 1. Dr. Chun-Yen Chen aligning the optics of the
atom trap used to count 81Kr atoms and demonstrate
the new Atom Trap Trace Analysis (ATTA) method. (Photo by George
Joch)
85Kr has a half-life of 10.8 years
and an isotope abundance of ~10-11 in the atmosphere,
while 81Kr has a half-life of 2.3 x 105
years and an abundance of 6 x 10-13. The
present-day 85Kr in the environment has been released
primarily by nuclear-fuel reprocessing plants. It has been used
as a general-purpose tracer to study air and ocean currents, date
shallow groundwater, and monitor nuclear-fuel reprocessing activities.
In contrast, 81Kr is produced in the upper atmosphere
by cosmic-ray induced reactions and is shielded from man-made
fission products by stable 81Br. 81Kr is
an ideal tracer for dating ancient groundwater and ice on the
time scale of 105-106 years. A method of
counting 81Kr atoms would also make possible a solar
neutrino detector that is sensitive to both 7Be and
8B neutrinos from the sun. |
Existing Methods
LLC [2] has generally been used to measure the
abundance of an isotope by counting its nuclear decays. It is
currently used to count 85Kr. Although once used to
count 81Kr, this is no longer possible because of the
high present-day decay background of 85Kr. Taking a
different approach, AMS [3] counts atoms instead of decays, thereby
greatly enhancing the detection efficiency and avoiding the radioactive
background problem. AMS is now routinely used as the standard
method of 14C-dating. Recently, AMS has been used to
count 81Kr and date groundwater [4]. In this work,
a large heavy-ion accelerator (K1200, MSU) was used to remove
all of the electrons from the atoms so that 81Kr can
be separated from its abundant isobar 81Br. |
 Figure 2. ATTA apparatus (about three meters long.
(a) Discharge Source; (b) Skimmer; (c) Transverse Cooling; (d)
Zeeman Slower; (e) Trap; (f) Photon Detector; (g) Balance Coil.).
In this work, a krypton gas sample is injected into the system
through a nozzle, around which a DC discharge is maintained. The
discharge excite a fraction of the atoms into the 5s[3/2]2
metastable level so that the atoms can be manipulated by laser
light at the convenient wavelength of 811nm. Two-dimensional transverse
cooling is used to reduce the atomic beam divergence and amplify
the atom flux in the forward di"RECT"ion. The thermal (300°C) atoms are then decelerated with the Zeeman slowing technique,
and loaded into a magneto-optical trap. A photo-diode viewing
the trap region detects the fluorescence of and count the trapped
atoms. |
Atom Trap Trace Analysis
A laser-based technique is attractive because it is simple, small
and inexpensive. ATTA is based on techniques of laser manipulation
of neutral atoms. In our system(see figure 2), individual krypton
atoms are trapped by laser light inside a vacuum chamber and detected
by viewing their fluorescence. An atom typically spends 0.1 second
in the trap and scatters one million photons. The sensitivity
of the fluorescence detector is such that a single trapped atom
provides a signal-to-noise ratio of 50 (see figure 3). |
 Figure
3. Single atom counting. (a) Signal showing the arrival and
departure of individual 83Kr atoms; (b) Signal of a single
trapped 81Kr atom. |
| For isotope separation, ATTA relies on the fact that different
types of atoms and molecules have different resonant frequencies.
Even different isotopes of the same element differ due to the so-called
isotope shifts. The atom trap is a wonderful isotope separator because
it only traps atoms of a particular isotope when the laser frequency
is tuned to its resonance position (see figure 4). |

Figure 4. Number of trapped krypton atoms versus laser
frequencies. (a) Dark peaks show the signals of abundant isotopes,
while the resonant frequencies of the rare isotopes are marked.
(b) Signal of the rare isotopes. The integration time of each data
point of 81Kr(85Kr) signal is 3 hours(0.5
hours). |
Applications
While the demonstration has been focused on krypton isotopes,
ATTA can be applied to many other trace-isotopes for a wide range
of potential applications including measuring solar neutrino flux,
searching for exotic particles, tracing atmospheric and oceanic
currents, archeological and geological dating, monitoring bone-loss
rates in the diagnosis of osteoporosis, and monitoring fission
products in the environment for safe-guarding nuclear wastes.
|
 Figure 5. Future applications of ATTA. (Illustration
by David Kurth) |
This work is currently pursued by a collaboration between the
Physics Division
(Kevin Bailey, Chun-Yen Chen, Xu Du, Yimin Li, Zheng-Tian Lu,
Tom O'Connor) and the Chemistry Division (Linda Young) of Argonne
National Laboratory. It is supported by the U.S. Department
of Energy, Nuclear Physics Division,
and LY by the Office of Basic Energy Sciences,
Division of Chemical
Sciences, under contract W-31-109-ENG-38.
Reference [1] C.Y. Chen et. al., Science 286, 1139 (1999).
[2] J.R. Arnold and W.F. Libby, Science 113, 111 (1951).
[3] R.A. Muller, Science 196, 489 (1977); D.E. Nelson
et. al., Science 198, 507 (1977); C.L. Bennett et. al.,
Science 198 508 (1977).
[4] P. Collon et. al., Nucl. Instr. and Meth. B123, 122
(1997); P. Collon, Ph.D. Thesis (University of Vienna, Austria
1999).
|
|
|