Effect of Xe bubble size and pressure on the thermal conductivity of UO2—A molecular dynamics study
Source abstract
Abstract
Thermal conductivity of uranium dioxide (UO2) is an important nuclear fuel performance property. Radiation- and fission-induced defects and microstructures, such as xenon (Xe) gas bubbles, can degrade the thermal conductivity of UO2significantly. Here, molecular dynamics simulations are conducted to study the effect of Xe bubble size and pressure on the thermal conductivity of UO2. At a given porosity, thermal conductivity increases with Xe cluster size, then reaches a nearly saturated value at a cluster radius of 0.6 nm, demonstrating that dispersed Xe atoms result in a lower thermal conductivity than clustering them into bubbles. In comparison with empty voids of the same size, Xe-filled bubbles lead to a lower thermal conductivity when the number ratio of Xe atoms to uranium vacancies (Xe:VUratio) in bubbles is high. Detailed atomic-level analysis shows that the pressure-induced distortion of atoms at bubble surface causes additional phonon scattering and thus further reduces the thermal conductivity.
Source: expertdata · Quality: candidate unverified · Source record ↗
Research context
OpenAlex topics: Nuclear Materials and Properties · Nuclear materials and radiation effects · Nuclear reactor physics and engineering
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (45)
Show source-provided references
1. 10.1016/0022-3115(83)90261-110.1016/0022-3115(83)90261-1 ↗
2. 10.1016/B978-0-08-056033-5.00039-210.1016/B978-0-08-056033-5.00039-2 ↗
3. 2015
4. 10.1103/PhysRevB.83.12520210.1103/PhysRevB.83.125202 ↗
5. 10.1016/S0022-3115(99)00273-110.1016/S0022-3115(99)00273-1 ↗
6. 10.1007/s10853-011-6230-010.1007/s10853-011-6230-0 ↗
7. 10.1016/j.jnucmat.2004.01.01810.1016/j.jnucmat.2004.01.018 ↗
8. 10.1016/j.nimb.2014.03.01810.1016/j.nimb.2014.03.018 ↗
9. J. Phys.: Condens. Matter · 2014 · 26 · 105401
10. 10.1016/0022-3115(88)90027-X10.1016/0022-3115(88)90027-X ↗
11. J. Phys.: Condens. Matter · 2016 · 28 · 405401
12. 10.1016/0022-3115(93)90229-R10.1016/0022-3115(93)90229-R ↗
13. 10.1016/j.jallcom.2007.03.03010.1016/j.jallcom.2007.03.030 ↗
14. 10.1016/0022-3115(88)90187-010.1016/0022-3115(88)90187-0 ↗
15. 10.1016/S0925-8388(03)00350-510.1016/S0925-8388(03)00350-5 ↗
16. Mater. Today · 2010 · 13 · 24
17. 10.1006/jcph.1995.103910.1006/jcph.1995.1039 ↗
18. 10.1063/1.47327110.1063/1.473271 ↗
19. 10.1103/PhysRevB.65.14430610.1103/PhysRevB.65.144306 ↗
20. 10.1016/j.ijheatmasstransfer.2016.03.10510.1016/j.ijheatmasstransfer.2016.03.105 ↗
21. 10.1016/0022-3115(71)90044-410.1016/0022-3115(71)90044-4 ↗
22. 10.1016/0022-3115(85)90352-610.1016/0022-3115(85)90352-6 ↗
23. 10.1016/0022-3115(85)90351-410.1016/0022-3115(85)90351-4 ↗
24. 10.1103/PhysRevB.85.14410210.1103/PhysRevB.85.144102 ↗
25. 10.1063/1.346293610.1063/1.3462936 ↗
26. 1976
27. 1881
28. 2016
29. 10.1016/j.jnucmat.2011.08.05210.1016/j.jnucmat.2011.08.052 ↗
30. 1992
31. 10.1016/B978-0-08-056033-5.00038-010.1016/B978-0-08-056033-5.00038-0 ↗
32. 10.1016/j.jnucmat.2011.02.04010.1016/j.jnucmat.2011.02.040 ↗
33. 10.1016/j.jnucmat.2014.05.03510.1016/j.jnucmat.2014.05.035 ↗
34. 10.1016/j.jnucmat.2012.11.04310.1016/j.jnucmat.2012.11.043 ↗
35. 10.1063/1.154394410.1063/1.1543944 ↗
36. 10.1016/j.jnucmat.2014.09.05210.1016/j.jnucmat.2014.09.052 ↗
37. 10.1016/S0168-583X(98)00040-810.1016/S0168-583X(98)00040-8 ↗
38. 10.1016/j.jnucmat.2015.12.02810.1016/j.jnucmat.2015.12.028 ↗
39. 10.1016/0022-3115(81)90575-410.1016/0022-3115(81)90575-4 ↗
40. 10.1103/PhysRevApplied.6.04401510.1103/PhysRevApplied.6.044015 ↗
41. 10.1016/j.jnucmat.2006.02.04710.1016/j.jnucmat.2006.02.047 ↗
42. 10.1016/j.jnucmat.2015.11.04210.1016/j.jnucmat.2015.11.042 ↗
43. 10.1063/1.498695610.1063/1.4986956 ↗
44. 10.1016/j.jnucmat.2015.03.03010.1016/j.jnucmat.2015.03.030 ↗
45. 10.3938/jkps.43.74710.3938/jkps.43.747 ↗