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Miller index : ウィキペディア英語版
Miller index

Miller indices form a notation system in crystallography for planes in crystal (Bravais) lattices.
In particular, a family of lattice planes is determined by three integers ''h'', ''k'', and ''ℓ'', the ''Miller indices''. They are written (hkℓ), and denote the family of planes orthogonal to h\mathbf + k\mathbf + \ell\mathbf, where \mathbf are the basis of the reciprocal lattice vectors. (Note that the plane is not always orthogonal to the linear combination of direct lattice vectors h\mathbf + k\mathbf + \ell\mathbf because the reciprocal lattice vectors need not be mutually orthogonal.) By convention, negative integers are written with a bar, as in for −3. The integers are usually written in lowest terms, i.e. their greatest common divisor should be 1.
There are also several related notations:〔Neil W. Ashcroft and N. David Mermin, Solid State Physics (Harcourt: New York, 1976)〕
*the notation denotes the set of all planes that are equivalent to (hkℓ) by the symmetry of the lattice.
In the context of crystal directions (not planes), the corresponding notations are:
*(), with square instead of round brackets, denotes a direction in the basis of the ''direct'' lattice vectors instead of the reciprocal lattice; and
*similarly, the notation ⟨hkℓ⟩ denotes the set of all directions that are equivalent to () by symmetry.
Miller indices were introduced in 1839 by the British mineralogist William Hallowes Miller. The method was also historically known as the Millerian system, and the indices as Millerian,〔(Oxford English Dictionary Online ) (Consulted May 2007)〕 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==

There are two equivalent ways to define the meaning of the Miller indices:〔 via a point in the reciprocal 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 vectors a1, a2, and a3 that define the unit cell (note that the conventional unit cell may be larger than the primitive cell of the Bravais lattice, as the examples below illustrate). Given these, the three primitive reciprocal lattice vectors are also determined (denoted b1, b2, and b3).
Then, given the three Miller indices h, k, ℓ, (hkℓ) denotes planes orthogonal to the reciprocal lattice vector:
: \mathbf_ = h \mathbf_1 + k \mathbf_2 + \ell \mathbf_3 .
That is, (hkℓ) simply indicates a normal to the planes in the basis 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 the ''shortest'' reciprocal lattice vector in the given direction.
Equivalently, (hkℓ) denotes a plane that intercepts the three points a1/''h'', a2/''k'', and a3/''ℓ'', or some multiple thereof. That is, the Miller indices are proportional to the ''inverses'' 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 (the ''lattice planes''), the perpendicular distance ''d'' between adjacent lattice planes is related to the (shortest) reciprocal lattice vector orthogonal to the planes by the formula: d = 2\pi / |\mathbf_|.〔
The related notation () denotes the ''direction'':
:h \mathbf_1 + k \mathbf_2 + \ell \mathbf_3 .
That is, it uses the direct lattice basis instead of the reciprocal lattice. Note that () is ''not'' generally normal to the (hkℓ) planes, except in a cubic lattice as described below.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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