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R. Kemp, G. Cottrell and H. K. D. H. Bhadeshia

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Presentation on theme: "R. Kemp, G. Cottrell and H. K. D. H. Bhadeshia"— Presentation transcript:

1 R. Kemp, G. Cottrell and H. K. D. H. Bhadeshia
A classical thermodynamic approach to void nucleation in irradiated materials R. Kemp, G. Cottrell and H. K. D. H. Bhadeshia University of Cambridge EPSRC, Culham Science Centre

2 Helium in irradiated materials
Alloy elements activated by neutron bombardment He created by a decay Sits at octahedral interstitial sites

3 Voids in irradiated materials
Voids formed from excess vacancies Require He to form BUT Not to grow (Cawthorne and Fulton, Nature 216 (1967)) Mansur L K, Journal of Nuclear Materials 216 (1994)

4 Void nucleation He moves into vacancies Can we model this as a bubble?
What is the equilibrium pressure? Adams and Wolfer, Journal of Nuclear Materials 166 (1989)

5 Gas potential Chemical potential per atom:

6 Solution potential Quasi-chemical model At equilibrium:
McLellan and Dunn, J. Phys. Chem. 30 (1969)

7 Equilibrium fugacity He = 1 appm

8 Steady state He concentration
Migration energy = eV Trapped at dislocations and in vacancies Need estimate of He concentration actually in solution Ghoniem et al, Journal of Nuclear Materials 117 (1983)

9 Steady state He concentration
He concentration of O(10-15 atom-1) QC effects significant from 10-9 atom-1 No contribution from QC model Equilibrium fugacity at atom-1 is O(1036 Pa) T / K Nominal 100 appm He

10 Summary “Equilibrium pressures” much greater than yield stresses
He may force creation of Frenkel pairs during desolution Nucleation must be dominated by available sites and arrival rates Assumption of fixed bubble density valid for many purposes


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