Lecture 25: The Liquid State Nucleation and Metallic Glasses - PowerPoint PPT Presentation

1 / 19
About This Presentation
Title:

Lecture 25: The Liquid State Nucleation and Metallic Glasses

Description:

Lecture 25: The Liquid State Nucleation and Metallic Glasses PHYS 430/603 material Laszlo Takacs UMBC Department of Physics – PowerPoint PPT presentation

Number of Views:105
Avg rating:3.0/5.0
Slides: 20
Provided by: Laszlo57
Category:

less

Transcript and Presenter's Notes

Title: Lecture 25: The Liquid State Nucleation and Metallic Glasses


1
Lecture 25 The Liquid State Nucleation and
Metallic Glasses
  • PHYS 430/603 material
  • Laszlo Takacs
  • UMBC Department of Physics

2
The states of matter
  • Gas - relatively simple
  • There is a reference state, the ideal gas, that
    can be understood in significant detail. Real
    gases are usually described as deviations from
    the ideal gas state due to interaction between
    molecules.
  • Crystalline solid - relatively simple
  • There is a reference state, the ideally periodic
    infinite crystal, that can be understood by
    focusing on the unit cell. Real crystals
    deviate from the ideal state due to finite
    crystallite size and defects.
  • Liquid - inherently complicated
  • There is no good reference state. Liquids are
    dense like solids with strong interaction between
    the molecules, but their structure is random, at
    least it has neither long range order nor unit
    cell. There is some short range order, both
    correlations in position and specific local
    geometries. The structure is dynamic, the
    molecules are in constant motion.
  • Intermediate cases
  • Amorphous materials - dense, random, but static
  • Quasicrystals - orientational order, but no
    periodicity
  • Partially ordered materials, e.g. liquid
    crystals

3
Structure from diffraction experiments
The intensity of the diffracted beam depends on
the phase difference between elementary rays
scattered by individual atoms.
  • Gas The relative atomic positions are random,
    constructive and destructive interference average
    out. Same as scattering by individual molecules.
  • Crystal If there is constructive interference
    between corresponding atoms in two neighboring
    unit cells, the interference is constructive
    between atoms from every unit cell, diffraction
    peak is observed.
  • Notice that XRD of crystals does not derive the
    structure from scratch, but only selects the
    structure from a list of possible structures
    allowed by symmetries. A 1-d (or possibly 2-d)
    measurement may not be able to reconstruct a 3-d
    structure.
  • Liquids and glasses There is some short range
    order and consequently an interference pattern,
    but only statistical information can be obtained
    from diffraction, the position of every atom
    cannot be determined.

4
Characterization of a liquid or amorphous
structure
  • Radial distribution function the probability of
    finding an atom at a distance r from an average
    atom.

For a completely random structure (gas) or for
large distances where there is no more short
range order, RDF approaches a parabola
corresponding to the average atomic density.
  • Notice that there is clear short-range order
  • The nearest neighbors are quite clearly defined,
    both their distance and their number (the area
    under the first peak.)
  • The second and third coordination shell are
    identifiable.
  • The curve approaches the 4?r2?0 parabola.
  • The bars indicate the distance and number of
    neighbors in crystalline hcp Zn. The short range
    order in the liquid is quite different - RDF
    cannot be obtained by broadening the crystalline
    distances.

5
What do we measure in diffraction?
  • Scattered intensity corrected for instrumental
    effects is the interference function, S(Q),
    where Q is the scattering vector (the change of
    the wave vector from the initial to the scattered
    state, Q 4?/? sin?.) From S(Q) the radial
    distribution function can be calculated
  • This seems to be a straightforward procedure, but
  • The interference function is known only to a
    finite Q, the integral must be truncated.
  • Instrumental effects must be considered very
    carefully, as the pattern consists of broad
    features, not sharp lines.

6
XRD results on amorphous FeP electrodeposited and
melt quenched alloys
  • Interference functions. Notice that the top three
    curves contain a small crystalline fraction. The
    lowest two define the fully amorphous
    concentration range, 16.7 to 22.9.
  • Hiltunen, Lehto, Takacs, 1986

RDF, P concentration increases down. Notice that
the short range order is similar but stronger
than in liquids. There is little variation
between samples, it is difficult to identify
trends.
7
Partial correlation functions for Ni60Nb40
  • The measured interference function is an average
    of the partial interference functions
    corresponding to the different atom pairs,
    weighted with the atomic scattering amplitudes.
    If three independent measurements with different
    scattering amplitudes are performed, the partial
    correlation functions can be separated.
  • The three measurements here were made using XRD,
    neutron diffraction with natural Ni and neutron
    diffraction on a sample made with 58Ni isotope.
  • Forgács, Hajdu, Sváb, J. Takács (1980)

8
Ni60Nb40 partial RDFs
  • There are clear differences between the curves,
    e.g. in the first neighbor distance and the shape
    of the split second peak. Unfortunately,
    decomposing similar curves from independent
    measurements, even different samples, results in
    large experimental uncertainties.
  • Another method of obtaining similar results is
    anomalous scattering of X-rays.

9
Crystallization
  • It is simple Over the melting point a material
    is liquid, below it is crystalline.
  • No! Starting to form a new phase also requires
    formation of a new interface!

10
  • Crystallization from the liquid state must always
    start from a nucleus.
  • Homogeneous nucleation from a cluster within the
    liquid.
  • Heterogeneous nucleation from a pre-existing
    surface, e.g. wall of the container or surface of
    impurity particle.

11
The free energy balance of homogeneous nucleation
Volume free energy Surface energy ?, assumed
to be direction independent For a spherical
nucleus of radius r
If r is small, the positive surface term
dominates, the formation of a small nucleus is
not favorable. But if a large nucleus forms
against the odds, for large r the negative volume
term dominates, the nucleus is stable. The two
regions are separated by the radius of the
critical nucleus
The volume energy gain increases with increasing
undercooling, consequently the critical radius
decreases, that is random fluctuations can more
easily - and more frequently -create a nucleus
larger than the critical size. At Tm the volume
energy gain becomes zero, the critical size
approaches infinity, there is no nucleation.
12
Heterogeneous nucleation
  • Nucleation can start at pre-existing surfaces,
    with substantial gain in surface energy. The most
    typical places for heterogeneous nucleation are
    the surface of the container and high-melting
    particles present in the melt (seeds added
    intentionally or impurities, e.g. oxides.)
  • Heterogeneous nucleation dominates close to the
    melting point, but homogeneous nucleation becomes
    important at low temperatures, as the number of
    heterogeneous nucleation sites is constant, but
    the number of homogeneous nuclei increases with
    decreasing temperature.
  • In order to achieve large undercooling,
    heterogeneous nucleation has to be avoided. The
    best is a small droplet with no room for a seed
    particle, levitated freely in a rf magnetic
    field. In industrial settings only a few degrees
    of undercooling take place, but 15 of Tm is
    possible in the laboratory.

13
The nucleation rate
  • The nucleation rate is proportional to the
    probability of forming a nucleus larger than
    critical size

Close to Tm the size and therefore the free
energy of the critical nucleus is large, the
nucleation rate is very slow, substantial
nucleation takes a very long time. At low
temperature, T in the denominator is small,
nucleation is slow because of the slow
dynamics. In between there is a degree of
undercooling where homogeneous nucleation is the
fastest. Growth is a diffusion-driven process
that has a rate according to the Fulcher equation
of
Finish Start
The fastest nucleation happens close to the
temperature a the tip of the curve.
Crystallization - can be avoided, by fast enough
cooling to avoid the nucleation line. This is how
metallic glasses are made.
The temperature variation of the nucleation and
growth rates explain the shape of the TTT -
time-temperature-transformation diagram.
14
What materials can form a glass?
  • Some materials - like mixtures of oxides,
    chalcogenides, complex organic materials - are
    easy glass formers. In those cases nucleation is
    very difficult because a large cluster of
    molecules must fit together by random motion to
    acct as a crystalline seed. Many of those
    materials do crystallize if cooling is very slow
    or seeds for heterogeneous nucleation are
    provided.
  • The structure of metals is simpler, thus
    nucleation is easier. Until 1959 it was believed
    that metals were always crystalline. This is not
    the case. Crystallization can be avoided also in
    metallic melts, if the difference between Tm and
    T0 is small. In a typical alloy system Tm can be
    strongly temperature dependent - deep eutectic
    points are advantegous - while T0 varies
    relatively little.
  • 1960 P. Duwez, Au-Si, later Pd-Si
  • Late 1960s The first ferromagnetic metallic
    glasses Fe80P12C8
  • 1975 The METGLAS 2605 family (Fe80B20 and
    related compositions)
  • Late 1970s Ni-Nb and other early-late transition
    metal systems
  • 1985-1995 a decade of decreasing interest
  • 1996 Inoue (Tohoku, Sendai) and W. Johnson
    (CalTech, Pasadena), bulk metallic glasses, such
    as Al-Y-Ni, La-Al-Ni Zr-Ni-Al-Cu, Zr-Ti-Cu-Ni-Be
    and Mg-Cu-Y

15
Some typical metallic glass forming systems
  • Au-Si the first one Fe-B ferromagnetic
    Nb-Ni metal-metal

16
Forming traditional metallic glasses requires
106 C/s cooling rate - possible only for thin
ribbons or sheets.Melt spinning is the most
frequently used method to reach such cooling
rates.
17
STM images of a crystalline and glassy Zr alloy
18
Mechanical property comparison for a bulk
metallic glass
19
Other subjects related to metallic glasses
  • Stability and crystallization
  • E.g. Fe(80)B(20) melt ? Fe(80)B(20) glass ? Fe
    Fe4B ? Fe Fe3B ? Fe Fe2B
  • Magnetism - no crystal structure, no
    magnetocrystalline anisotropy, stress sensitivity
    can be minimized by varying the composition
  • E.g. (Fe1-xCox)75Si15B10 at about x 0.9
  • Partially crystallized magnetically hard-soft
    alloys.
  • Other materials produced by rapid quenching
    Quasicrystals, metastable compounds
Write a Comment
User Comments (0)
About PowerShow.com