scholarly journals Longevity of Plutonium 238 Heat Sources

2012 ◽  
Vol 1444 ◽  
Author(s):  
Roberta N. Mulford ◽  
Paul D. Richardson ◽  
Joseph Hickey ◽  
Rene Chavarria

ABSTRACTPlutonium oxide heat sources are used to power space missions. The heat produced by alpha decay of the 238 isotope of Pu is converted to electricity in a thermopile, providing electricity during a substantial fraction of the 88 year half-life of the isotope. Decay of the Pu produces helium and uranium, and a fraction of the evolved helium is captured in the oxide matrix. All of the helium produced in decay can in principle be contained in the oxide lattice, where it occupies the tetrahedral sites. Some helium diffuses out at a rate that is somewhat dependent on the form and morphology of the fuel. Rates have previously been measured for oxide aged about 1 year. Current measurements on sealed heat sources as old as 34 years indicate that the rate of diffusion has changed only slightly over time. Possible mechanisms for helium release include bubble diffusion, point defect migration, agglomeration and movement of He at grain boundaries, and volume diffusion through the lattice sites. We observe primarily diffusion from site to site within the lattice, with an activation energy of 18.7 kcal/mole, independent of point defect movement, despite the rising concentration of helium in the lattice over time and the accumulation of radiation damage within the lattice. Because of the slow diffusion of helium from the fuel to the headspace, heat sources are anticipated to be stable over a long lifetime.

Mineral grains from three depths within the Luna 24 drill core ( ca . 90, 125 and 196 cm) have been examined for solar-flare tracks. Large proportions (55-100%) of grains from all three levels are found to be track-rich (with central track densities p e > 10 8 cm -2 ), and a substantial fraction ( ca . 25-50%) of all grains display trackdensity gradients. These observations indicate that most of the mineral grains have been cycled through the top ca . 1 mm of the lunar surface at some time in their history. Some degree of submaturity is observed towards the bottom of the core. The most likely depositional model envisages rapid infall of highly irradiated material into a less mature local component with rather little subsequent reworking. Thermoluminescence (t.l.) studies indicate a lower natural radiation dose in samples from the 196 cm level compared with those from the two upper levels. This can result either from random variations in the local internal radioactivity or from mixing properties of the pre-irradiated material over time scales of less than ca . 100 ka. Radiation sensitization of samples suggests a possible use of t.l. sensitivity for the interpretation of lunar radiation history.


PAMM ◽  
2006 ◽  
Vol 6 (1) ◽  
pp. 439-440
Author(s):  
Oliver Goy ◽  
Ralf Mueller ◽  
Dietmar Gross

1998 ◽  
Vol 538 ◽  
Author(s):  
L. R. Corrales ◽  
R.M. Van Ginhoven ◽  
J. Song ◽  
H. Jónsson

AbstractA study of vacancy defect migration pathways and energetics in a-quartz is carried out using an empirical simulation methodology that is coupled with the nudged elastic band method. Results from this study indicate that the migration pathway for migration is between adjacent sites. We anticipate the results will guide modifications to empirical potentials for use in the study of point defect formation of more complex systems.


2001 ◽  
Vol 82-84 ◽  
pp. 207-212 ◽  
Author(s):  
Sebania Libertino ◽  
Salvatore Coffa

2005 ◽  
Vol 12 (04) ◽  
pp. 493-498
Author(s):  
EMAD A. BADAWI

The trapping of positrons at vacancy site in some materials provide a new and sensitive method for the equilibrium determination of point defect migration enthalpy. Data are presented for commercial Al–Mg alloys and fitted to a model allowing presentation in the form of Arrhenius plots, hence the migration enthalpy [Formula: see text] can be determined by positron annihilation lifetime technique (PALT). The results show that as the concentration of Mg increases the value of [Formula: see text] increases too.


2014 ◽  
Vol 891-892 ◽  
pp. 452-457 ◽  
Author(s):  
Jaroslav Polák ◽  
Jiří Man

Cyclic plastic straining in crystalline materials is localized to persistent slip bands (PSBs) and results in formation of persistent slip markings (PSMs) consisting of extrusions and intrusions. Intensive plastic strain in PSBs results in dislocation interactions and formation of point defects. The extended model based on point defect formation, migration and annihilation is presented describing surface relief formation in the form of extrusion-intrusion pairs. Point defect migration and resulting mass transfer is the principle source of cyclic slip irreversibility leading to crack-like defects - intrusions. Fatigue cracks start in the tip of sharp intrusions.


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