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Miller index

From Wikipedia, the free encyclopedia
Notation system for crystal lattice planes
Planes with different Miller indices in cubic crystals
Examples of directions

Miller indices form a notation system incrystallography for lattice planes incrystal (Bravais) lattices.

In particular, a family oflattice planes of a given (direct)Bravais lattice is determined by threeintegersh,k, and , theMiller indices. They are written (hkℓ), and denote the family of (parallel) lattice planes (of the given Bravais lattice) orthogonal toghk=hb1+kb2+b3{\displaystyle \mathbf {g} _{hk\ell }=h\mathbf {b} _{1}+k\mathbf {b} _{2}+\ell \mathbf {b} _{3}}, wherebi{\displaystyle \mathbf {b} _{i}} are thebasis orprimitive translation vectors of thereciprocal lattice for the given Bravais lattice. (Note that the plane is not always orthogonal to the linear combination of direct or original lattice vectorsha1+ka2+a3{\displaystyle h\mathbf {a} _{1}+k\mathbf {a} _{2}+\ell \mathbf {a} _{3}} because the direct lattice vectors need not be mutually orthogonal.) This is based on the fact that a reciprocal lattice vectorg{\displaystyle \mathbf {g} } (the vector indicating a reciprocal lattice point from the reciprocal lattice origin) is the wavevector of a plane wave in the Fourier series of a spatial function (e.g., electronic density function) which periodicity follows the original Bravais lattice, so wavefronts of the plane wave are coincident with parallel lattice planes of the original lattice. Since a measured scattering vector inX-ray crystallography,Δk=koutkin{\displaystyle \Delta \mathbf {k} =\mathbf {k} _{\mathrm {out} }-\mathbf {k} _{\mathrm {in} }} withkout{\displaystyle \mathbf {k} _{\mathrm {out} }} as the outgoing (scattered from a crystal lattice) X-ray wavevector andkin{\displaystyle \mathbf {k} _{\mathrm {in} }} as the incoming (toward the crystal lattice) X-ray wavevector, is equal to a reciprocal lattice vectorg{\displaystyle \mathbf {g} } as stated by theLaue equations, the measured scattered X-ray peak at each measured scattering vectorΔk{\displaystyle \Delta \mathbf {k} } is marked byMiller indices.

By convention,negative integers are written with a bar, as in3 for −3. The integers are usually written in lowest terms, i.e. theirgreatest common divisor should be 1. Miller indices are also used to designate reflections inX-ray crystallography. In this case the integers are not necessarily in lowest terms, and can be thought of as corresponding to planes spaced such that the reflections from adjacent planes would have a phase difference of exactly one wavelength (2π), regardless of whether there are atoms on all these planes or not.

There are also several related notations:[1]

In the context of crystaldirections (not planes), the corresponding notations are:

Note, for Laue–Bragg interferences

Miller indices were introduced in 1839 by the British mineralogistWilliam Hallowes Miller, although an almost identical system (Weiss parameters) had already been used by German mineralogistChristian Samuel Weiss since 1817.[2] The method was also historically known as the Millerian system, and the indices as Millerian,[3] although this is now rare.

The Miller indices are defined with respect to any choice of unit cell and not only with respect to primitive basis vectors, as is sometimes stated.

Definition

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Examples of determining indices for a plane using intercepts with axes; left (111), right (221)

There are two equivalent ways to define the meaning of the Miller indices:[1] via a point in thereciprocal lattice, or as the inverse intercepts along the lattice vectors. Both definitions are given below. In either case, one needs to choose the three lattice vectorsa1,a2, anda3 that define the unit cell (note that the conventional unit cell may be larger than the primitive cell of theBravais lattice, as theexamples below illustrate). Given these, the three primitive reciprocal lattice vectors are also determined (denotedb1,b2, andb3).

Then, given the three Miller indicesh,k,,(hk){\displaystyle h,k,\ell ,(hk\ell )} denotes planes orthogonal to the reciprocal lattice vector:

ghk=hb1+kb2+b3.{\displaystyle \mathbf {g} _{hk\ell }=h\mathbf {b} _{1}+k\mathbf {b} _{2}+\ell \mathbf {b} _{3}.}

That is, (hkℓ) simply indicates a normal to the planes in thebasis of the primitive reciprocal lattice vectors. Because the coordinates are integers, this normal is itself always a reciprocal lattice vector. The requirement of lowest terms means that it is theshortest reciprocal lattice vector in the given direction.

Equivalently, (hkℓ) denotes a plane that intercepts the three pointsa1/h,a2/k, anda3/, or some multiple thereof. That is, the Miller indices are proportional to theinverses of the intercepts of the plane, in the basis of the lattice vectors. If one of the indices is zero, it means that the planes do not intersect that axis (the intercept is "at infinity").

Considering only (hkℓ) planes intersecting one or more lattice points (thelattice planes), the perpendicular distanced between adjacent lattice planes is related to the (shortest) reciprocal lattice vector orthogonal to the planes by the formula:d=2π/|ghk|{\displaystyle d=2\pi /|\mathbf {g} _{hk\ell }|}.[1]

The related notation [hkℓ] denotes thedirection:

ha1+ka2+a3.{\displaystyle h\mathbf {a} _{1}+k\mathbf {a} _{2}+\ell \mathbf {a} _{3}.}

That is, it uses the direct lattice basis instead of the reciprocal lattice. Note that [hkℓ] isnot generally normal to the (hkℓ) planes, except in a cubic lattice as described below.

Cubic structures

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For the special case of simple cubic crystals, the lattice vectors are orthogonal and of equal length (usually denoteda), as are those of the reciprocal lattice. Thus, in this common case, the Miller indices (hkℓ) and [hkℓ] both simply denote normals/directions inCartesian coordinates.

For cubic crystals withlattice constanta, the spacingd between adjacent (hkℓ) lattice planes is (from above)

dhk=ah2+k2+2{\displaystyle d_{hk\ell }={\frac {a}{\sqrt {h^{2}+k^{2}+\ell ^{2}}}}}.

Because of the symmetry of cubic crystals, it is possible to change the place and sign of the integers and have equivalent directions and planes:

  • Indices inangle brackets such as ⟨100⟩ denote afamily of directions which are equivalent due to symmetry operations, such as [100], [010], [001] or the negative of any of those directions.
  • Indices incurly brackets orbraces such as {100} denote a family of plane normals which are equivalent due to symmetry operations, much the way angle brackets denote a family of directions.

Forface-centered cubic andbody-centered cubic lattices, the primitive lattice vectors are not orthogonal. However, in these cases the Miller indices are conventionally defined relative to the lattice vectors of the cubicsupercell and hence are again simply the Cartesian directions.

Hexagonal and rhombohedral structures

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Hexagonal Miller–Bravais indices for the (1121) plane

Forhexagonal andrhombohedrallattice systems, theBravais–Miller system is typically used, which uses four indices (hki) that obey the constraint

h +k +i = 0.

Hereh,k and are identical to the corresponding Miller indices, andi is a redundant index.

This four-index scheme for labeling planes in a hexagonal lattice makes permutation symmetries apparent. For example, the similarity between (110) ≡ (1120) and (120) ≡ (1210) is more obvious when the redundant index is shown.

In the figure at right, the (001) plane has a 3-fold symmetry: it remains unchanged by a rotation of 1/3 (2π/3 rad, 120°). The [100], [010] and the [110] directions are really similar. IfS is the intercept of the plane with the [110] axis, then

i = 1/S.

There are alsoad hoc schemes (e.g. in thetransmission electron microscopy literature) for indexing hexagonallattice vectors (rather than reciprocal lattice vectors or planes) with four indices. However they do not operate by similarly adding a redundant index to the regular three-index set.

For example, the reciprocal lattice vector (hkℓ) as suggested above can be written in terms of reciprocal lattice vectors ashb1+kb2+b3{\displaystyle h\mathbf {b} _{1}+k\mathbf {b} _{2}+\ell \mathbf {b} _{3}}. For hexagonal crystals this may be expressed in terms of direct-lattice basis-vectorsa1,a2 anda3 as

hb1+kb2+b3=23a2(2h+k)a1+23a2(h+2k)a2+1c2()a3.{\displaystyle h\mathbf {b} _{1}+k\mathbf {b} _{2}+\ell \mathbf {b} _{3}={\frac {2}{3a^{2}}}(2h+k)\mathbf {a} _{1}+{\frac {2}{3a^{2}}}(h+2k)\mathbf {a} _{2}+{\frac {1}{c^{2}}}(\ell )\mathbf {a} _{3}.}

Hence zone indices of the direction perpendicular to plane (hkℓ) are, in suitably normalized triplet form, simply[2h+k,h+2k,(3/2)(a/c)2]{\displaystyle [2h+k,h+2k,\ell (3/2)(a/c)^{2}]}. Whenfour indices are used for the zone normal to plane (hkℓ), however, the literature often uses[h,k,hk,(3/2)(a/c)2]{\displaystyle [h,k,-h-k,\ell (3/2)(a/c)^{2}]} instead.[4] Thus as you can see, four-index zone indices in square or angle brackets sometimes mix a single direct-lattice index on the right with reciprocal-lattice indices (normally in round or curly brackets) on the left.

And, note that for hexagonal interplanar distances, they take the form

dhk=a43(h2+k2+hk)+a2c22{\displaystyle d_{hk\ell }={\frac {a}{\sqrt {{\tfrac {4}{3}}\left(h^{2}+k^{2}+hk\right)+{\tfrac {a^{2}}{c^{2}}}\ell ^{2}}}}}
However, in general:
dhkl=2πh2b12+k2b22+l2b32+2hkb1b2cosγ+2klb2b3cosα+2lhb1b3cosβ{\displaystyle d_{hkl}={\frac {2\pi }{\sqrt {h^{2}{\textbf {b}}_{1}^{2}+k^{2}{\textbf {b}}_{2}^{2}+l^{2}{\textbf {b}}_{3}^{2}+2hk{\textbf {b}}_{1}{\textbf {b}}_{2}\cos \gamma ^{*}+2kl{\textbf {b}}_{2}{\textbf {b}}_{3}\cos \alpha ^{*}+2lh{\textbf {b}}_{1}{\textbf {b}}_{3}\cos \beta ^{*}}}}}

Crystallographic planes and directions

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Dense crystallographic planes

Crystallographic directions arelines linking nodes (atoms,ions ormolecules) of a crystal. Similarly, crystallographicplanes areplanes linking nodes. Some directions and planes have a higher density of nodes; these dense planes have an influence on the behavior of the crystal:

  • optical properties: in condensed matter,light "jumps" from one atom to the other with theRayleigh scattering; thevelocity of light thus varies according to the directions, whether the atoms are close or far; this gives thebirefringence
  • adsorption andreactivity: adsorption and chemical reactions can occur at atoms or molecules on crystal surfaces, these phenomena are thus sensitive to the density of nodes;
  • surface tension: the condensation of a material means that the atoms, ions or molecules are more stable if they are surrounded by other similar species; the surface tension of an interface thus varies according to the density on the surface
  • dislocations (plastic deformation)
    • the dislocation core tends to spread on dense planes (the elastic perturbation is "diluted"); this reduces thefriction (Peierls–Nabarro force), the sliding occurs more frequently on dense planes;
    • the perturbation carried by the dislocation (Burgers vector) is along a dense direction: the shift of one node in a dense direction is a lesser distortion;
    • the dislocation line tends to follow a dense direction, the dislocation line is often a straight line, a dislocation loop is often apolygon.

For all these reasons, it is important to determine the planes and thus to have a notation system.

Non-integer Miller indices

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Ordinarily, Miller indices are always integers by definition, and this constraint is physically significant. To understand this, suppose that we allow a plane (abc) where the Miller "indices"a,b andc (defined as above) are not necessarily integers.

Lattice planes

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Ifa,b andc haverational ratios, then the same family of planes can be written in terms of integer indices (hkℓ) by scalinga,b andc appropriately: divide by the largest of the three numbers, and then multiply by theleast common denominator. Thus, integer Miller indices implicitly include indices with all rational ratios. The reason why planes where the components (in the reciprocal-lattice basis) have rational ratios are of special interest is that these are thelattice planes: they are the only planes whose intersections with the crystal are 2d-periodic.

Quasicrystals

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For a plane (abc) wherea,b andc haveirrational ratios, on the other hand, the intersection of the plane with the crystal isnot periodic. It forms an aperiodic pattern known as aquasicrystal. This construction corresponds precisely to the standard "cut-and-project" method of defining a quasicrystal, using a plane with irrational-ratio Miller indices. (Although many quasicrystals, such as thePenrose tiling, are formed by "cuts" of periodic lattices in more than three dimensions, involving the intersection of more than one suchhyperplane.)

See also

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References

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  1. ^abcAshcroft, Neil W.; Mermin, N. David (1976).Solid state physics. New York: Holt, Rinehart and Winston.ISBN 0030839939.OCLC 934604.
  2. ^Weiss, Christian Samuel (1817)."Ueber eine verbesserte Methode für die Bezeichnung der verschiedenen Flächen eines Krystallisationssystems, nebst Bemerkungen über den Zustand der Polarisierung der Seiten in den Linien der krystallinischen Structur".Abhandlungen der physikalischen Klasse der Königlich-Preussischen Akademie der Wissenschaften:286–336.
  3. ^Oxford English Dictionary Online (Consulted May 2007)
  4. ^J. W. Edington (1976)Practical electron microscopy in materials science (N. V. Philips' Gloeilampenfabrieken, Eindhoven)ISBN 1-878907-35-2, Appendix 2

External links

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