Pu-loaded glasses and crystals: evolution due to self-irradiation
Shiryaev A.A.
Frumkin Institute of Physical chemistry and electrochemistry RAS, Moscow
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Pu-loaded glasses and crystals: evolution due to self-irradiation Shiryaev A.A. Frumkin Institute of Physical chemistry and electrochemistry RAS, Moscow With contributions by: B.E. Burakov, S.V. Stefanovsky, V.O. Yapaskurt and many other
Frumkin Institute of Physical chemistry and electrochemistry RAS, Moscow
Isotope Activity (microCi/(microgram)) 230Th 0.1/(5) 232Th 100/(900 grams) 233U 1/(100) 235U 1/(50000) 238U 100/(300 grams) 237Np 0.1/(140) 238Pu 0.1/(0.006) 239Pu 0.1/(0.03) 244Cm 0.1/(0.001)
2500 g 239Pu
238Pu
(Eu,Pu)PO4 monazite doped with 4.9 wt% 238Pu, grown in
At ~1.1x1018 decays/gram dispersed particles has appeared; at ~5.2x1018 decays/gram “peeling” has started.
Images: B.E. Burakov
He range ≤ n·10 µm U range ~ n·10 nm
µm
Al2O3 B2O3 Gd2O3 HfO2 La2O3 Nd2O3 PuO2 SiO2 SrO
200 400 600 800 1000
10000 20000 30000 40000
760 780 800 820 840 860 880 900 920 940 1000 2000 3000 4000 5000 6000 7000 8000Intensity Channels
Pu
Identified phases (XRD+SEM/EDX)
PuO2: crystallites with sizes of >50 nm. Solid solution
(Pu,Hf)O2 with a fluorite structure (SEM/EDX/XRD) Britholite: (approx. REE10Si6O24(OH)2) is a “real” powder.
10 20 30 40
2 , degrees
Young (1 year storage) Old (1.5 year storage)
PuO2
1000 2000 3000
Intensity, arb. units
Raman shift, cm-1
(mostly Q2 units)
shell shows similarity to PuO2+x (PuO2.2?)
phase.
the first sphere becomes more pronounced. In the fresh glass it comprises two subspheres, whereas for the 2 y.o. glass – three (similar to Conradson et al., JACS, 126, 13443, 2004).
1 2 3 4 5 6
FT Magnitude R, A
1 year storage 1.5 years storage
Sample Atom Distance, А Occupation 2 y.o. glass О 1.87-1.92 0.15-0.47 О 2.09-2.12 ~1.2 О 2.20-2.27 4±1 Pu 3.74 2±0.5 Fresh glass О 2.13 1.3 О 2.25-2.28 5 Pu 3.66-3.69 2.5±0.5
FT peak of the first coordination shell is asymmetric – superposition
contributions from various phases.
5 10 15 20 1 2 3 4
REE or Hf(?)
Pu
k, A-1 R, A
0.02925 0.05850 0.08775 0.1170 0.1463 0.1755 0.2048 0.2340
O
5 10 15 20 1 2 3 4
k, A-1
R, A
0.1687 0.3375 0.5062 0.6750 0.8437 1.013 1.181 1.350
5 10 15 20 1 2 3 4
k, A-1
R, A
0.04213 0.08425 0.1264 0.1685 0.2106 0.2528 0.2949 0.3370
5 10 15 20
1 2 3 4
k, A-1
R, A
0.2750 0.5500 0.8250 1.100 1.375 1.650 1.925 2.200
space indicates better separation of contributions from glassy and crystalline phases.
and britholite grains are precipitated, the grain size and crystallographic perfection increases.
1 2 3 4 5 6
R, A
Hafnium L3
200 400 600 800 1000 1200 1400 1600 1800 2000
Intensity, arb. units
Raman shift, cm-1 Frit 1 high Hf, low Al and Si Frit 3 Frit 4 Frit 5 low Hf, high Al and Si
Raman scattering
5 10 15 20 1.0 1.5 2.0 2.5 3.0 3.5 4.0
k, A-1 R, A
0.06675 0.1335 0.2003 0.2670 0.3337 0.4005 0.4672 0.53405 10 15 20 1.0 1.5 2.0 2.5 3.0 3.5 4.0
R, A
0.07000 0.1400 0.2100 0.2800 0.3500 0.4200 0.4900 0.5600Silicates
Precipitates of (Pu, Hf)O2 solid solution and of REE-Al phase!! Dendritic morphology consistent with CaF2-structural type dendrites Exsolution (rapid?) of excess PuO2?
Formation of altered layer, which may crack and detach from underlying bulk Rather uniform process on the whole glass surface
Infra-red spectroscopy shows presence of OH-groups in (Zr, U)O2 and in chernobylite (not in UO2!) Moisture-induced spontaneous transition of tetragonal zirconia to monoclinic phase is accompanied by considerable volume increase: possible mechanism
the lava cracking.
Undissolved fuel pellet? UO2 precipitated from the melt always contains Zr admixture
Variable morphology :
α-tra racks:
10 min 2h
Particle size: 200x100 μm!
Wt % O 39 Na 26 S 15 U 10
0.00 1.00 2.00 3.00 4.00 5.00 6.00 7.00 8.00 9.00 10.00 keV 022 150 300 450 600 750 900 1050 1200 1350 1500 1650 1800 1950 Counts
O Na Mg Al Si S S Cl Cl K K Ca Ca Zr Zr U U U U
Image by R.E.Williford, PNNL
18000 18100 18200 18300 18400 0,0 0,2 0,4 0,6 0,8 1,0 1,2 1,4 1,6 1,8
Absorption
E, eV
Be
Images: B.E. Burakov
5 10 15 20 1 2 3 4 5 6
k, A-1
R, A
1 2 3 4 5 6
FT magnitude
R, A
S.G. P 21/n a = 6.3864(11) Å α = γ = 90 b = 6.8668(12) Å β = 104.028(7) c = 6.6654(11) Å V = 283.59(8) Å3 Slow swelling with accumulated dose…
17150 17200 17250 17300
0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6
Absorption
Energy, eV
Recoil U might be hexavalent
200 300 400 500 600 700 800 900 1000 1100 1200
Raman shift. cm-1
Bulk "Blister" "Blister" burned Non-active EuPO4
900 925 950 975 1000 1025 1050
Bulk "Blister" burned "Blister" Non-active EuPO4
Raman shift. cm-1
C
Excitation 785 nm Excitation 532 nm
500 520 540 560 580 600 620 640 660 680 700
Wavelength, nm
Bulk+"Blister"
"Blister" Bulk Non-active EuPO4
300 nm 120 nm
40 nm 10 nm
300 nm
4.11 Å (100) 3.06 Å (20-2) 1.8 Å 1.7 Å
Reflections from misoriented crystallites
300 nm
Transport of Plutonium in the Far-Field of the Mayak Production Association, Russia. Science, 2006
Prokofiev V.Yu., et al., Fluid inclusions with colloid solutions in chalcedony, TBG XIII Proceedings (2009) Prokofiev V.Yu., et al., Geology, 2017
13 days at 150 °C
Relatively pristine nanospheres AND numerous nm-sized particles with high Z-contrast – Pu compounds?
Partly destroyed spheres. Diffraction shows presence of crystallites (reprecipitated SiO2?). Treatment at 70 °C gives similar results
Rather small amount of degraded nanospheres is found. Pu-rich particles are also present.
n*10-1000 nm 5-20 nm
100 nm 100 nm
Shiryaev et al., Sci.Rep., 2018
At a “selected” ratio of ion energy and grain size the grains are completely destroyed!