Diat Htt Lect 4 5 6

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    HeatTreatment

    Dr.SantoshS.Hosmani

    III. Grain-size / Grain-boundary hardening, fgb:

    12

    = n

    N

    at 100X magnification

    nASTM grain size number

    645 dGrain diameter inmeters101 10)2(

    n nASTM grain size number

    49

    V. Solid solution hardening, fss:

    Mixture of two or more metals

    Solute atoms: a zero dimensional defect or a point defect

    Two types:

    1. Interstitial solid solution

    .

    50

    V. Solid solution hardening, fss:

    Interstitial Solid Solution

    Perfect Cr stal Distortion caused by a

    large interstitial atom

    51

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    V. Solid solution hardening, fss:

    Substitutional Solid Solution

    Small solute atom Large solute atom

    Solute atom: a zero-dimensional point defect52

    V. Solid solution hardening, fss:

    Strains in theSolute

    Obstacle to dislocationStrong

    Alloys stronger than pure metals53

    V. Solid solution hardening, fss:

    annealed ferrite

    Here, factors affecting hardness are:

    Size difference between solute

    and solvent atoms,

    Elastic modulus of solute

    54

    V. Solid solution hardening, fss:

    This conce t is relevant to allo desi n

    55

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    IV. Precipitation Hardening, fppt:

    This conce t is directl relevant to heat-

    treatment of alloys, e.g. ???

    56

    IV. Precipitation Hardening, fppt:

    Hardness increases as a function of time.

    Al-Cu alloys:

    In 1906 Alfred Wilm a metallurgist working

    at Dren in Germany quenched an

    experimental AlCu-alloy after annealing it and

    left the specimen on the bench over the

    weekend. Testing it a few days later heeekend. Testing it a few days later he

    found that both hardness and strength had

    increased simply by having been left at room

    t t W l th D lemperature. Wilm gave the name Duralumin

    to his alloys after the place where they were

    first made.

    Alfred WilmBorn: June 25, 1869

    Died: August 6, 1937

    IV. Precipitation Hardening, fppt:

    Hardness increases as a function of time.

    Al-Cu alloys:

    As-quenched

    As-quenched

    hardness

    Ref.: Book by D.A. Porter, & K.E. Easterling 58

    IV. Precipitation Hardening, fppt:

    59

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    IV. Precipitation Hardening, fppt:

    b =

    64 65Ref.: Book by D.A. Porter, & K.E. Easterling

    Lattice misfit =>

    66Volume misfit =>

    Ref.: Book by D.A. Porter, & K.E. Easterling

    Misfit strain energy:

    67Ref.: Book by D.A. Porter, & K.E. Easterling

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    68Ref.: Book by D.A. Porter, & K.E. Easterling 69Ref.: Book by D.A. Porter, & K.E. Easterling

    70

    Ref.: Book by D.A. Porter, & K.E. Easterling

    Thermodynamics & Kinetics aspects for aging process

    G

    0Q

    Greactants

    Gdriving force =

    G1+G2+G3+G4 4+

    Gproducts

    Reaction state

    The activation ener barrier to the

    formation of each transition phase (i.e.

    & ) is very small in comparison to the

    barrier against the direct precipitation of

    71

    e equ r um p ase .e. u2

    Ref.: Book by D.A. Porter, & K.E. Easterling

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    Thermodynamics & Kinetics aspects for aging process

    Figure: Schematic diagram showing the total free energy of the alloy versus time

    72

    Ref.: Book by D.A. Porter, & K.E. Easterling

    Thermodynamics & Kinetics aspects for aging process

    73

    Ref.: Book by D.A. Porter, & K.E. Easterling

    Figure: Hardness as

    time for an Al-4Cu

    alloy.

    Transmission electron micrographs:

    74

    Thermodynamics & Kinetics aspects for aging process

    Why / How precipitates coarsen by consuming other precipitates?

    75Figure:Schematic illustration of formation ofprecipitates in the matrix (a

    and b) and their coarsening (c to f)

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    Thermodynamics & Kinetics aspects for aging process

    Why / How precipitates coarsen by consuming other precipitates?

    76

    Ref.: Book by D.A. Porter, & K.E. Easterling

    Although cold-rolled and annealed sheet steels have

    Strain Aging

    ,

    close to the A1 temperature, some carbon and nitrogen

    are always taken into solution (unless the steels areultralow-carbon or interstitialfree steels). Figure shows

    are carbon-rich side of the Fe-C diagram. Carbon has

    its maximum solubility at the A1 temperature, and itssolubility decreases with temperature to a negligible

    .

    relationship. Thus, if a steel is cooled from around A1

    at a rate that prevents gradual relief of supersaturationby cementite formation during cooling, the ferrite at

    room temperature may e g y supersaturate w t

    respect to carbon and nitrogen. These interstitial

    elements then may segregate to dislocations in

    strained structures a rocess referred to as strain

    aging, or they may precipitate out as fine carbide ornitride particles, a process referred to as quenchaging. The aging processes may occur at room

    77

    empera ure or urng ea ng a empera ures us

    above room temperature because of the high diffusivity

    of carbon and nitrogen in the bcc ferrite structure.

    IV. Precipitation Hardening, fppt:

    Movement of one-dimensional defects

    called dislocations causes plastic

    Obstacles to the movement of

    dislocations cause strengthening

    78

    Howtointroducetheobstaclestothemotionofdislocations?

    II. other dislocations giving what is calledWork Hardening (fwh),

    III. grain boundaries introducingGrainsize Hardening (fgb),

    IV.precipitates or dispersed particles giving Precipitation

    Hardening (fppt),

    V. by adding alloying elements to give Solid Solution Hardening

    ss .

    These techniques for manipulating strength are central

    to alloy design.79

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    80