Effect of heavy ion irradiation dose rate and temperature on a' precipitation in high purity Fe-18%Cr alloy
Creators
- 1. University of Tennessee, Knoxville, TN 37996 (United States)
- 2. Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831 (United States)
- 3. INSA de Rouen Normandie, Avenue de l'universite, 76801 St Etienne du Rouvray, (France)
- 4. Groupe de Physique des Materiaux, UMR 6634 CNRS, Universite de Rouen Normandie (France)
- 5. Center for Nanophase Materials Science (CNMS), Oak Ridge National Laboratory, Oak Ridge, TN 37831 (United States)
- 6. CEA, DEN, Service de Recherches Metallurgiques Appliquees, Laboratoire d'Analyse Microstructurale des Materiaux, Universite Paris-Saclay F-91191 Gif-sur-Yvette, (France)
Description
Cr-rich alpha prime precipitates (CrRP) induce hardening and embrittlement of FeCr alloys, but the kinetics of CrRP formation due to particle irradiation are not well understood. In this study, Fe18wt.%Cr alloy in solid solution state and pre-aged to produce relatively coarse CrRP was irradiated with 8 MeV Fe ions. The irradiation conditions involved two midrange doses of 0.37 and 3.7 displacements per atom (dpa), a wide range of dose rates (10(-5)-10(-3) dpa/s) and temperatures (300-450 degrees C). The distributions of CrRP after irradiation were studied with atom probe tomography (APT). The critical irradiation conditions to suppress CrRP formation were identified as 300 degrees C and 10(-3) dpa/s; CrRP formation occurred readily at lower dose rates or higher temperatures. From 0.37 to 3.7 dpa, CrRP were observed to slightly grow at 350 degrees C and strongly coarsen at 450 degrees C. Specimens with pre-existing CrRP evolved into a similar precipitate distribution as detected after ion irradiation on solution annealed specimens at 300-350 degrees C to 0.37 dpa, indicating that the precipitate microstructure approaches a quasi-equilibrium for doses < 1 dpa. Limited shrinking of pre-existing CrRP was observed after irradiation at 450 degrees C to 0.37 dpa, indicating a higher recovery rate at this temperature. The evolution of CrRP is quantitatively explained by employing corrections to the historic Nelson-Hudson-Mazey precipitate stability model, and a radiation modified precipitation mechanism is proposed to account for the competition between radiation enhanced diffusion and ballistic dissolution which results in the modifications on both size and solute concentration of CrRP. (authors)
Availability note (English)
Available from doi: http://dx.doi.org/10.1016/j.actamat.2022.117888Additional details
Identifiers
Publishing Information
- Journal Title
- Acta Materialia
- Journal Volume
- 231
- Journal Page Range
- p. 117888.1-117888.17
- ISSN
- 1359-6454
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- France
- INIS RN
- 56001357
- Subject category
- S36: MATERIALS SCIENCE;
- Descriptors DEI
- AGING; CHROMIUM ALLOYS; DISSOLUTION; DOSE RATES; EMBRITTLEMENT; HARDENING; HEAVY IONS; IRON ALLOYS; IRON IONS; IRRADIATION; MICROSTRUCTURE; PRECIPITATION; PRECIPITATION HARDENING; PROBES; SOLID SOLUTIONS; TOMOGRAPHY
- Descriptors DEC
- ALLOYS; CHARGED PARTICLES; DIAGNOSTIC TECHNIQUES; DISPERSIONS; HARDENING; HOMOGENEOUS MIXTURES; IONS; MIXTURES; SEPARATION PROCESSES; SOLUTIONS; TRANSITION ELEMENT ALLOYS
Optional Information
- Notes
- 94 refs.