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NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

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NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard
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Page 1: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

NEEP 541 – Radiation Damage in Steels

Fall 2002Jake Blanchard

Page 2: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Outline Damage in Steels

Page 3: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Steels in Reactors Requirements

High temperature operation High strength Inexpensive Low corrosion

Page 4: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Steel Types Austenitic

Primarily austenite phase - FCC Stabilized by Ni Good creep strength Resists corrosion with sodium and

mixed oxide fuels Inexpensive High void swelling

Page 5: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

CompositionElement 304 (wt %) 316 (wt %)

Fe 70 65

Cr 19 17

Ni 9 13

C .06 .06

Mn .8 1.8

P .02 .02

S .02 .02

Si .5 .3

B .0005 .0005

N .03

Mo .2 2.2

Co .2 .3

Page 6: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Steel Types Ferritic Steels

Primarily ferrite – BCC Cheaper than austenitic steels Susceptible to DBTT increases

Page 7: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

CompositionElement A 302-B A 212-B

Fe 97 98

C .2 .3

Mn 1.3 .8

P .01 .01

Si .3 .3

S .02 .02

Cr .2 .2

Ni .2 .2

Mo .5 .02

Page 8: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.
Page 9: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Microstructure Evolution Transmission Electron Microscopy is

used to study damage Several hundred keV electron beam

passes through sample Some electrons transmitted, others

diffracted Only transmitted electrons are viewed Defects alters diffraction conditions When defects are oriented to transmit

better, then they appear as a dark image

Page 10: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Black Dot Structure Defects produced at low

temperatures show up on TEM as black dots

Defects are too small to be resolved They are believed to be depleted

zones or small vacancy clusters Below 350 C, increased fluence

increases black dot density

Page 11: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Other structures Above 350 C, point defects are

mobile Loops become predominant Voids also form

Page 12: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Microstructure of Unirradiated SS

Page 13: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Loops in Irradiated SS

Page 14: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Voids in SS

Page 15: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Hardening of Austenitic Steels Low Fluence

Hardening primarily from depleted zones

At low T (below half the melting temperature), little annealing, hardening occurs

At high T, damage anneals out, no hardening

Page 16: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Hardening of Austenitic Steels High Fluence

Loops and Voids grow Annealing is slower

Page 17: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

316 SS

Page 18: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

316 SS

Page 19: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Steel Type Affects Damage Large differences exist among

various types and heat treatments Weld metal is often more

susceptible than base metal Even a single type of steel can

exhibit large variations in damage effects

Page 20: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Transition Temp. for different batches of steel

Page 21: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Differences due to structure Damage differences can result

from: grain size, texture, etc. Saturation of damage can also be

sensitive to microstructure

Page 22: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Saturation

Page 23: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Chemistry Chemistry may be the most important

factor in steel embrittlement Sulphur and phosphorous are

detrimental Irradiation can form sulfides (MnS,

FeS) These nucleate segregation of copper Adding N leads to increased

hardening, either by forming clusters or collecting in loops

Page 24: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Effect of radiation on DBTTin steel containing Cu

Page 25: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

316 SS, 400 C, 130 dpa

Page 26: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Helium Some steels have B in them B has a high He production cross

section He can lead to embrittlement

Page 27: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

He Production Cross Sections

Page 28: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Damage in pure Fe Pure iron: defects are

Small black spots (small loops or planar clusters)

Loops cavities

Page 29: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Neutron Damage Must have fluence>4x1023 n/m2

Threshold is lower for less pure metals

At low fluence, defect distribution is heterogeneous

Clusters and loops are only formed near dislocations or sub-boundaries

Page 30: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Damage in a low-carbon steel At 275-450 C, cavities observed Sizes are up to 12 nm in diameter Concentration up to 1021 /m3

Above 500 C, cavities only at grain boundaries

No cavities at all above 575 C

Page 31: NEEP 541 – Radiation Damage in Steels Fall 2002 Jake Blanchard.

Annealing Annealing pure Fe below 300 C has

no effect on black dots Annealing above 300 C leads to

loops Above 500 C, loops are annealed

away


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