Fundamentals of Radiation Damage- Lecture 4 Flashcards
The two categories of damage
1. The primary damage that is formed immediately (within a few picoseconds) after the ion/neutron/electron impact by atomic collision processes.
2. The long-time scale (nanoseconds to years) damage evolution caused by thermally activated processes.
Where does energy come from for dynamic and thermal annealing?
Dynamic: energy from interactions (collisions)
Thermal: energy from heat in the system (reactor operating temperatures)
How can larger and more stable extended defects form?
Point defects can agglomerate to form larger, more stable defects. Examples are interstitials combining with interstitials to form an interstitial type dislocation or vacancies combining with vacancies to form a vacancy type dislocation
What happens when defect density reaches a critical level?
Amorphisation occurs.
What plays an important role in recovery/accumulation?
Temperature during irradiation
Types of damage that may remain after irradiation
Vacancies/interstitials
Dislocation loops
Voids and gas bubbles
Phase separation/formation (redistribution of alloy metal elements)
Amorphisation
Why is it surprising that irradiated materials swell?
Vacancy dislocation loops should reduce the volume of a material. Interstitial dislocation loops should increase volume. In general we expect compensating vacancy and interstitial effects to leave the material with approximately the same volume. But irradiated materials do swell
How do cavities form?
Accumulation of vacancy type dislocation loops
Why do irradiated alloys swell?
Absorption of neutrons by the elements can cause transmutation into unstable isotopes that decay by alpha decay. The alpha particles then pick up electrons in the metal to for He atoms. He atoms stabilise cavities. Cavities grow by further acquisition of vacancies and eventually approach a size and distribution that is sufficient to effect macroscopic change in the apparent bulk volume of the alloy. Void nucleation and growth occurs between 0.3+0.5 Tm and He gas can escape to leave cavities empty
Compare the swelling rates of austenitic and ferritic/martensitic steels
Swelling rate is increase in ΔV/V0 with dpa.
Austenitic: FCC, initial slow swelling rate, then about 1%/dpa swelling rate, graph looks like exponential increase.
Ferritic/martensitic: 0.2%/dpa swell rate, swelling resistance due to BCC crystal structure and complicated defect-sink interactions
Comparison of visible defect cluster accumulation in BCC vs FCC regions of stainless steel after irradiation
BCC has much fewer and a bit larger visible defect clusters under a microscope than FCC.
Difference in size distributions of dislocation loops for irradiated BCC and FCC stainless steel
BCC (like δ ferrite) has wider variation in size of dislocation loops whereas FCC has them more concentrated at lower sizes. FCC also has more dislocation per unit volume than BCC under same irradiation conditions
How does gas bubble formation occur?
Alpha particle is a He nucleus which picks up electrons to form a He atom. Reactor core temperatures (like 600°C) allow He atom migration and agglomeration into bubbles
What are the bubble-like features that arise in fuel pellets?
The empty region of the bubble contains the gaseous fission products. The smaller filled region of a different colour is the metal fission products.
Xe concentration profile across a fuel pellet cross section
Is close to 0 at and near the centre. Then steep curves up further away from centre, then flat for a bit and just before the edges very sharply down a bit