novel temporal gamma spectroscopy … · research were supported by the inl internship program 1...
TRANSCRIPT
Oregon State University | College of Engineering | School of Nuclear Science and Engineering
NOVEL TEMPORAL GAMMA SPECTROSCOPY INSTRUMENTATION AND ANALYTICAL METHODS IN DETERMINING PHOTOFISSION PRODUCT YIELDS
ABSTRACTDespite the decades of previous research, many aspects of the available, empirical fission data are lacking. The evaluated data widely used in
computational tools suffer from inaccuracies and large relative uncertainties, particularly with respect to short-lived and low-yield fission products.
The existing data is often based on nuclear models and limited experimental measurements of these fission product yields have been performed. This
work seeks to validate and improve, where applicable, the current fission product yield data in the ENDF library using experimental measurements,
particularly for the fission of U-238 and Th-232 .
A reliable way to determine composition of radioactive materials is through the measurement and analysis of delayed gamma rays emitted from the
decay of fission products. High-purity germanium (HPGe) detectors, with standard and altered preamplifiers, are being employed for measurements
of short-lived fission products, collecting data between accelerator pulses in irradiations of U-238 and Th-232. One of the challenges associated with
measuring low-yield, short-lived fission products is the inability of commercial detectors and data acquisition systems to operate quickly, efficiently,
and in high-flux environments - a necessity for such measurements. In previous measurements, much of the measurable fission products would have
decayed away during sample transfer from the linear accelerator (linac) to the measurement setup. This results in low count rates and large
uncertainty in the calculated yield of fission products, especially for the short-lived ones.
This work leverages previous research examining pulse processing algorithms for high-throughput, high-resolution spectroscopy and the comparison
of measured and simulated delayed gamma ray spectra following photofission. Using established nuclear codes (e.g. ORIGEN-S and MCNP) delayed
gamma ray spectra will be simulated and compared to our measurement results. The quality and precision of data in the existing library, as
determined from this comparison, will be evaluated and reported.
Ari Foley a, Dr. Haori Yang a, Dr. Mathew Kinlaw b
a School of Nuclear Science and Engineering, Oregon State University, Corvallis, OR 97331, USA, b Idaho National Laboratory, Idaho Falls, ID 83415, USA
60 80 100 120 140 160
10-2
10-1
100
101
DT Fission
(14 MeV neutrons)
Fra
ctional m
ass y
ield
Mass number
Fast Fission
(500 keV neutrons)
Photofission
Figure 1: Fractional mass yields produced by DT neutron fission, photofission (,f) (22 MeV); and fast neutron fission (500 KeV) of 238U.1,2
INTRODUCTIONNeutrons and photons can excite a nucleus and cause fission in nuclear materials. Following a fission event, emitted signals can be
measured for detection and identification purposes. Exploitable signatures can be based on neutrons and photons, both prompt and
delayed. Delayed gamma rays are more abundant, long-lasting, and are often easier to detect following a fission event. A unique gamma
ray intensity distribution exists for each fissionable isotope allowing material identification.
One of the challenges associated with measuring low-yield, short-lived fission products is the inability of commercial detectors and data
acquisitions systems to operate quickly, efficiently, and in high-flux environments, a necessity for such measurements. Similar
requirements exist for practical security and safeguards applications which rely upon observing and characterizing fission signatures in
order to detect and identify special nuclear material. Increasing the throughput capabilities—the amount of information the acquisition
system can process without loss—and limiting the processing time required for those measurements is of paramount importance.
Balancing the processing time inherent to those detection systems with the need for sufficient measurement precision requires
advancement to the current state of the art.
MOTIVATION➢ Improved nuclear data for isotopes of interest in SNM detection and nuclear forensics
➢ Photonuclear isotope production methods for nuclear forensics projects
Aluminum Beam ScrubPhoton Radiator
e-
Beam Exit Aluminum Beam ScrubPhoton Radiator
e-
Beam Exit
Figure 2: (left) MCNP6 mesh tally of electron beam into photon radiator (left, red/blue) (Right) Tally of electron beam (red/blue) with resulting photon spectrum (purple/yellow)
Figure 3: Experimental setup with pneumatic shuttle for irradiations in linac hall with the 25 MeV accelerator at the Idaho Accelerator Center in February 2018
ACKNOWLEDGEMENTThis research was performed using funding received from the DNDO Academic Research Initiative Program and portions of thisresearch were supported by the INL internship program
1England, T. R. and Rider, B. R.; “Evaluation and Compilation of Fission Product Yields,” ENDF-349, LA-UR-94-3106, Los Alamos National Laboratory (1994)2Belyshev, S. S., Ishkhanov, A. A. and Stopani, K. A.; “Mass yield distributions and fission modes in photofission of 238U below 20 MeV,” Phys Rev C 91, 034603 (2015).
EXPERIMENTAL SETUPTwo separate experimental setups have been tested: one with both modified and standard HPGe detectors facing the sample in an
experimental hall, adjacent to the linac hall, with a collimated photon beam from the 90 degree port, and the other utilizing a
pneumatic shuttle and the HPGe located within the linac hall during operation. Maximizing count rates while preventing loss in
energy resolution is a delicate balance. The intensity of the produced signal has a prompt drop following the end of an individual
accelerator pulse and an increasing amount of information is lost the later that measurement begins.
ANALYSESIn order to observe products with the lowest relative yields, cycles of irradiation and counting periods will be required. Custom software (coupling ORIGEN-S and MCNP6) is used in conjunction with MCNP6 simulations to determine
the optimal combination of counting and irradiation cycles. Measurements are analyzed to extract independent yields of the short-lived fission products based on Levenberg-Marquardt least squares fitting algorithms specific to the
isotope of interest’s decay chain.
Figure 4: Example of measured gamma spectrum from 0 to 8 seconds of irradiated U-238 at 22 MeV
Figure 5: Gamma spectrum signature of isotope of interest, Zr-99 (Data from Figure 5)
Figure 6: Illustration of decomposition of the peaks (at 469 keVand 465 keV) contributing to bulk peak
0 1 2 3 4
0
2
4
Figure 7: Scope trace to visualize timing of linac charge measured by faraday target (yellow), HPGe preamp signal (cyan), and the “magic pulse” (magenta) to pneumatic
rabbit
Time (400 ms/div)
Lin
acC
har
ge (
Yello
w)
1 V
ver
tica
l sca
le;
HP
Ge
pre
amp
(cy
an)
sign
al 2
00
mV
ver
tica
l sca
le;
Mag
ic P
uls
e (m
agen
ta)
1 V
ver
tica
l sca
le.
Horizontal for all is 400 ms per division on scope: 4 us total range
200 400 600 800 1000 1200
100
200
300
400
500
Co
un
ts
Photon energy (keV)
2-4 sec
6-8 sec
360 380 400 420 440 460 480 500
100
200
Co
un
ts
Photon energy (keV)
2-4 sec
6-8 sec
469 keV 99Zr
2 3 4 5 6 7 8 9 10 11 120
20
40
60
80
100
120
140
160
180
469
keV
rate
(s
-1)
Time (s)
Bateman Eq for Zr-99
430 440 450 460 470 480
100
200
Counts
Photon energy (keV)
2-4 sec
6-8 sec
Figure 7: Yield from 594 keV peak to verify Zr-99 peak against known half-life (Using data from Figure 6)