Graeme Ackland March 2010 Elasticity and Plasticity Graeme Ackland University of Edinburgh.
-
Upload
ryan-wilson -
Category
Documents
-
view
237 -
download
0
Transcript of Graeme Ackland March 2010 Elasticity and Plasticity Graeme Ackland University of Edinburgh.
Graeme AcklandMarch 2010
Elasticity and Plasticity
Graeme AcklandUniversity of Edinburgh
Graeme AcklandMarch 2010
ceiiinossssttuu (Hooke 1675) Ut tensio, sic vis i.e. linear response of stress to strain
Tensor quantities Nine Components 3 rotations 1 volume 5 shears
Graeme AcklandMarch 2010
Strain There are two definitions of strain
Engineering strain = L /Lo ; = F / Ao
True strain = ln(L / Lo); = F / A
Both depend on a reference state.
Graeme AcklandMarch 2010
Cubic materials - elasticity
81 ratios between 9 shears and 9 strains.
Notation, e.g. xyxy = 66; xxyy = 12
C12 = xx/yy
Symmetry reduces this considerably. E.g.
2: Shear and bulk moduli (homogenous material)
3: C12, C11 C44 (cubic)
5: C11 C33 C12 C13 C44 (hexagonal)
Graeme AcklandMarch 2010
Calculation of elastic moduli
Second derivative of the free energy.
Apply a strain, calculate stress tensor.
Apply a special strain, calculate energy.
Practical concern: Even at 0K, atoms may change their positions in response to shear.
Relax the atoms
Elastic moduli drop significantly with temperature
Graeme AcklandMarch 2010
Actual deformation modes Not all elastic moduli correspond
to appliable strains: in cubic B=(C11+2C12) / 3 C’= C11-C12 / 2 C44
These combinations must be positive: the Born Stability Criteria
Graeme AcklandMarch 2010
Harmonic Phonons: Free energy
Calculate the energy as a function of small displacements
(second term is zero at equilibrium). Create a matrix equation of motion
The eigenvalues of this dynamical matrix are the phonon energies,
eigenvectors are the phonon modes. They are independent harmonic oscillators.
Graeme AcklandMarch 2010
Harmonic Free energy
Once the phonon frequencies are known, the temperature-dependent free energy is just statistical mechanics (Born & Huang etc.)
(neglects phonon-phonon interactions, anharmonicity, thermal expansion)
Unless … One of the eigenvalues is negative.Which it is in -Ti
Graeme AcklandMarch 2010
Dynamical stability
Negative phonon eigenvalue means
Energy goes down as structure distorts
Crystal structure is UNSTABLE at T=0
Can define phonon by curvature of the energy, or by autocorrelation function (MD).
In practice, there is always some limit to the phonon modulations.
Graeme AcklandMarch 2010
Phonon modes in Zr (similar to Ti)
Phonon dispersion curve at 1400 K. Dashed lines: MD calculation
Circles are neutron scattering results
Solid lines quasiharmonic lattice-dynamics calculations for perfect bcc
Imaginary frequencies corresponding to unstable phonons are shown as negative.
Graeme AcklandMarch 2010
Dislocations
An extra half plane of atoms creating a line defect
Graeme AcklandMarch 2010
Dislocations
Characterised by:
Burgers vector
the plane, how much slip you get
Glide Plane
Plane swept out by the line as it moves
Screw, edge or mixed.
Graeme AcklandMarch 2010
Dislocation Mobility
Small burgers vectors move more easily.
Intermetallic compounds are hard.
Obstacles can hold up dislocations (precipitates, impurities, other dislocations)
More on dislocations tomorrow…
Graeme AcklandMarch 2010
Dislocation simulation
In modelling, dislocations are treated in three ways:
Molecular dynamics: explicit atom geometry
Dislocation dynamics: simulation of interacting lines
Finite element: unspecified source of plasticity
Graeme AcklandMarch 2010
Five slip systems: a counting exercise
A unit cell is defined by a parallelipiped, three vectors, a 3x3 matrix.
Nine degrees of freedom Three rotations One dilatation (volume)So to deform to a general shape requiresthe remaining five to be slip systems
Graeme AcklandMarch 2010
Creep and Climb (QT movies)
Dislocations cannot move in the plane of the extra half plane without adding atoms.
This is climb, depends on vacancy migration and stress.
Very slow, but requires only low stresses to bias vacancies arriving vs leaving.
Not restricted to a particular slip system.
Graeme AcklandMarch 2010
Deformation Twinning - Micrographs
Fast, large shear, no long range strain :
High activation energy
easy to calculate twin boundary energy
Graeme AcklandMarch 2010
Martensitic Twins: Cycling
Damage Accumulates, defects store memory.
Austenite energy
Martensite energy
Martensite Structure
Graeme AcklandMarch 2010
An MD simulation of a dislocation (bcc iron)
Starting configuration
Periodic in xy, fixed layer of atoms top and bottom in z
Dislocation in the middle
Move fixed layers to apply stress
Final Configuration (n.b. periodic boundary)
Dislocation has passed through the material
many times: discontinuity on slip plane
Graeme AcklandMarch 2010
Molecular dynamics simulation of twin and dislocation deformation