Published 2016
| Version v1
Journal article
Growth rate effects on the formation of dislocation loops around deep helium bubbles in Tungsten
- 1. Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Description
Here, the growth process of spherical helium bubbles located 6 nm below a (100) surface is studied using molecular dynamics and parallel replica dynamics simulations, over growth rates from 106 to 1012 helium atoms per second. Slower growth rates lead to a release of pressure and lower helium content as compared with fast growth cases. In addition, at slower growth rates, helium bubbles are not decorated by multiple dislocation loops, as these tend to merge or emit given sufficient time. At faster rates, dislocation loops nucleate faster than they can emit, leading to a more complicated dislocation structure around the bubble.
Availability note (English)
Available from http://www.osti.gov/pages/biblio/1334150Additional details
Additional titles
- Augmented title (English)
- KEYWORDS: MATERIAL SCIENCE; MAGNETIC FUSION ENERGY; HELIUM BUBBLES; DISLOCATION LOOP PUNCHING; PARALLEL REPLICA DYNAMICS
Identifiers
Publishing Information
- Journal Title
- Fusion Science and Technology
- Journal Volume
- 71
- Journal Issue
- 1
- Journal Page Range
- 7 p.
- ISSN
- 1536-1055
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 48018305
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- BUBBLES; COMPUTERIZED SIMULATION; DISLOCATIONS; HELIUM; MOLECULAR DYNAMICS METHOD; NUCLEATION; SPHERICAL CONFIGURATION
- Descriptors DEC
- CALCULATION METHODS; CONFIGURATION; CRYSTAL DEFECTS; CRYSTAL STRUCTURE; ELEMENTS; FLUIDS; GASES; LINE DEFECTS; NONMETALS; RARE GASES; SIMULATION
Optional Information
- Contract/Grant/Project number
- AC52-06NA25396
- Funding organization
- USDOE Office of Science - SC. Advanced Scientific Computing Research (ASCR) (SC-21) (United States)
- Secondary number(s)
- LA-UR--16-21485; OSTIID--1334150