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Helium Bubbles in Fe: Equilibrium Configurations and Modification by Radiation

Published online by Cambridge University Press:  21 February 2013

Xiao Gai
Affiliation:
Mathematical Sciences Department, Loughborough University, Leicestershire, LE11 3TU, UK
Roger Smith
Affiliation:
Mathematical Sciences Department, Loughborough University, Leicestershire, LE11 3TU, UK
Steven Kenny
Affiliation:
Mathematical Sciences Department, Loughborough University, Leicestershire, LE11 3TU, UK
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Abstract

We have examined the properties of helium bubbles in Fe using two different Fe-He potentials. The atomic configurations and formation energies of different He-vacancy complexes are determined and their stability in the region of nearby collision cascades is investigated. The results show that the optimal He to Fe vacancy ratio increases from about 1:1 for approximately 5 vacancies up to about 4:1 for 36 vacancies. Collision cascades initiated near the complex show that Fe vacancies produced by the cascades readily become part of the He-vacancy complexes. The energy barrier for an isolated He interstitial to diffuse was found to be 0.06 eV. Thus a possible mechanism for He bubble growth would be the addition of vacancies during a radiation event followed by the subsequent accumulation of mobile He interstitials produced by the corresponding nuclear reaction.

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Articles
Copyright
Copyright © Materials Research Society 2013 

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References

REFERENCES

Zinkle, S. J., Phys. Plasmas, 12(2005) 058101.10.1063/1.1880013CrossRefGoogle Scholar
Lucas, G., Schäublin, R., J. Phys.: Condens. Mater, 20(2008) 415206.Google Scholar
Stoller, R. E., Golubov, S. I., Kamenski, P. J., Seletskaia, T., Osetsky, Yu. N., Phil. Mag. 90(2010) 923934.10.1080/14786430903298768CrossRefGoogle Scholar
Gao, F., Deng, Huiqiu, Heinisch, H. L., Kurtz, R. J., J. Nucl. Mater. 418(2011) 115120.10.1016/j.jnucmat.2011.06.008CrossRefGoogle Scholar
Ackland, G. J., Bacon, D. J., Calder, A. F. and Harry, T., Phil. Mag. A 75(1997) p.713.10.1080/01418619708207198CrossRefGoogle Scholar
Ackland, G. J., Mendelev, M. I., Srolovitz, D. J., Han, S., Barashev, A. V., J. Phys.: Condens. Mater, 16(2004) S2629.Google Scholar
Aziz, R. A., Janzen, A. R., Moldover, M. R., Phys. Rev. Lett. 74(1995) 1586.10.1103/PhysRevLett.74.1586CrossRefGoogle Scholar
Miller, M. K., Russell, K. F., Pareige, P., Starink, M. J., Thomson, R. C., Mater. Sci. Eng. A 250(1998) 49.10.1016/S0921-5093(98)00535-8CrossRefGoogle Scholar
Auger, P., Pareige, P., Welzel, S., van Duysen, J-C., J. Nucl. Mater. 280(2000) 331344.10.1016/S0022-3115(00)00056-8CrossRefGoogle Scholar
Henkelman, G., Jónsson, H., J. Chem. Phys. 111(1999) 7010.10.1063/1.480097CrossRefGoogle Scholar
Fu, C. C., Willaime, F., Phys. Rev. B 72(2005) 064117.10.1103/PhysRevB.72.064117CrossRefGoogle Scholar