He migration and bubble formation in Ga stabilised delta-Pu

The migration and formation of He into bubbles in Ga stabilised δ-Pu has been investigated using molecular dynamics simulation. Formation energy calculations indicate that isolated He interstitial atoms are unfavourable and that it is preferential for He to reside as a substitutional atom at the exp...

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Main Authors: Robinson, Marc, Kenny, S., Smith, R., Storr, M.
Format: Journal Article
Published: Elsevier BV * North-Holland 2014
Online Access:http://hdl.handle.net/20.500.11937/25676
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author Robinson, Marc
Kenny, S.
Smith, R.
Storr, M.
author_facet Robinson, Marc
Kenny, S.
Smith, R.
Storr, M.
author_sort Robinson, Marc
building Curtin Institutional Repository
collection Online Access
description The migration and formation of He into bubbles in Ga stabilised δ-Pu has been investigated using molecular dynamics simulation. Formation energy calculations indicate that isolated He interstitial atoms are unfavourable and that it is preferential for He to reside as a substitutional atom at the expense of producing a Pu self-interstitial. Migration energy barrier calculations and on-the-fly kinetic Monte Carlo simulations support this result establishing that an interstitial He atom soon becomes substitutional, after which migration is unlikely unless assisted by local vacancies. He-vacancy cluster formation energies show that as the void size increases, a He:vacancy ratio up to 2:1 becomes energetically favourable over isolated He substitutional atoms and vacancies.
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institution Curtin University Malaysia
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publishDate 2014
publisher Elsevier BV * North-Holland
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spelling curtin-20.500.11937-256762017-09-13T15:16:05Z He migration and bubble formation in Ga stabilised delta-Pu Robinson, Marc Kenny, S. Smith, R. Storr, M. The migration and formation of He into bubbles in Ga stabilised δ-Pu has been investigated using molecular dynamics simulation. Formation energy calculations indicate that isolated He interstitial atoms are unfavourable and that it is preferential for He to reside as a substitutional atom at the expense of producing a Pu self-interstitial. Migration energy barrier calculations and on-the-fly kinetic Monte Carlo simulations support this result establishing that an interstitial He atom soon becomes substitutional, after which migration is unlikely unless assisted by local vacancies. He-vacancy cluster formation energies show that as the void size increases, a He:vacancy ratio up to 2:1 becomes energetically favourable over isolated He substitutional atoms and vacancies. 2014 Journal Article http://hdl.handle.net/20.500.11937/25676 10.1016/j.jnucmat.2013.10.017 Elsevier BV * North-Holland unknown
spellingShingle Robinson, Marc
Kenny, S.
Smith, R.
Storr, M.
He migration and bubble formation in Ga stabilised delta-Pu
title He migration and bubble formation in Ga stabilised delta-Pu
title_full He migration and bubble formation in Ga stabilised delta-Pu
title_fullStr He migration and bubble formation in Ga stabilised delta-Pu
title_full_unstemmed He migration and bubble formation in Ga stabilised delta-Pu
title_short He migration and bubble formation in Ga stabilised delta-Pu
title_sort he migration and bubble formation in ga stabilised delta-pu
url http://hdl.handle.net/20.500.11937/25676