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Structure factor

From Wikipedia, the free encyclopedia
Mathematical description in crystallography

Incondensed matter physics andcrystallography, thestatic structure factor (orstructure factor for short) is a mathematical description of how a material scatters incident radiation. The structure factor is a critical tool in the interpretation of scattering patterns (interference patterns) obtained inX-ray,electron andneutrondiffraction experiments.

Confusingly, there are two different mathematical expressions in use, both called 'structure factor'. One is usually writtenS(q){\displaystyle S(\mathbf {q} )}; it is more generally valid, and relates the observed diffracted intensity per atom to that produced by a single scattering unit. The other is usually writtenF{\displaystyle F} orFhk{\displaystyle F_{hk\ell }} and is only valid for systems with long-range positional order — crystals. This expression relates the amplitude and phase of the beam diffracted by the(hk){\displaystyle (hk\ell )} planes of the crystal ((hk){\displaystyle (hk\ell )} are theMiller indices of the planes) to that produced by a single scattering unit at the vertices of theprimitive unit cell.Fhk{\displaystyle F_{hk\ell }} is not a special case ofS(q){\displaystyle S(\mathbf {q} )};S(q){\displaystyle S(\mathbf {q} )} gives the scattering intensity, butFhk{\displaystyle F_{hk\ell }} gives the amplitude. It is themodulus squared|Fhk|2{\displaystyle |F_{hk\ell }|^{2}} that gives the scattering intensity.Fhk{\displaystyle F_{hk\ell }} is defined for a perfect crystal, and is used in crystallography, whileS(q){\displaystyle S(\mathbf {q} )} is most useful for disordered systems. For partially ordered systems such ascrystalline polymers there is obviously overlap, and experts will switch from one expression to the other as needed.

The static structure factor is measured without resolving the energy of scattered photons/electrons/neutrons. Energy-resolved measurements yield thedynamic structure factor.

Derivation ofS(q)

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Consider thescattering of a beam of wavelengthλ{\displaystyle \lambda } by an assembly ofN{\displaystyle N} particles or atoms stationary at positionsRj,j=1,,N{\displaystyle \textstyle \mathbf {R} _{j},j=1,\,\ldots ,\,N}. Assume that the scattering is weak, so that the amplitude of the incident beam is constant throughout the sample volume (Born approximation), and absorption, refraction and multiple scattering can be neglected (kinematic diffraction). The direction of any scattered wave is defined by its scattering vectorq{\displaystyle \mathbf {q} }.q=ksko{\displaystyle \mathbf {q} =\mathbf {k_{s}} -\mathbf {k_{o}} }, whereks{\displaystyle \mathbf {k_{s}} } andko{\displaystyle \mathbf {k_{o}} } (|ks|=|k0|=2π/λ{\displaystyle |\mathbf {k_{s}} |=|\mathbf {k_{0}} |=2\pi /\lambda }) are the scattered and incident beamwavevectors, andθ{\displaystyle \theta } is the angle between them. For elastic scattering,|ks|=|ko|{\displaystyle |\mathbf {k} _{s}|=|\mathbf {k_{o}} |} andq=|q|=4πλsin(θ/2){\displaystyle q=|\mathbf {q} |={{\frac {4\pi }{\lambda }}\sin(\theta /2)}}, limiting the possible range ofq{\displaystyle \mathbf {q} } (seeEwald sphere). The amplitude and phase of this scattered wave will be the vector sum of the scattered waves from all the atomsΨs(q)=j=1NfjeiqRj{\displaystyle \Psi _{s}(\mathbf {q} )=\sum _{j=1}^{N}f_{j}\mathrm {e} ^{-i\mathbf {q} \cdot \mathbf {R} _{j}}}[1][2]

For an assembly of atoms,fj{\displaystyle f_{j}} is theatomic form factor of thej{\displaystyle j}-th atom. The scattered intensity is obtained by multiplying this function by its complex conjugate

I(q)=Ψs(q)×Ψs(q)=j=1NfjeiqRj×k=1NfkeiqRk=j=1Nk=1Nfjfkeiq(RjRk){\displaystyle I(\mathbf {q} )=\Psi _{s}(\mathbf {q} )\times \Psi _{s}^{*}(\mathbf {q} )=\sum _{j=1}^{N}f_{j}\mathrm {e} ^{-i\mathbf {q} \cdot \mathbf {R} _{j}}\times \sum _{k=1}^{N}f_{k}\mathrm {e} ^{i\mathbf {q} \cdot \mathbf {R} _{k}}=\sum _{j=1}^{N}\sum _{k=1}^{N}f_{j}f_{k}\mathrm {e} ^{-i\mathbf {q} \cdot (\mathbf {R} _{j}-\mathbf {R} _{k})}}1

The structure factor is defined as this intensity normalized by1/j=1Nfj2{\displaystyle 1/\sum _{j=1}^{N}f_{j}^{2}}[3]

S(q)=1j=1Nfj2j=1Nk=1Nfjfkeiq(RjRk){\displaystyle S(\mathbf {q} )={\frac {1}{\sum _{j=1}^{N}f_{j}^{2}}}\sum _{j=1}^{N}\sum _{k=1}^{N}f_{j}f_{k}\mathrm {e} ^{-i\mathbf {q} \cdot (\mathbf {R} _{j}-\mathbf {R} _{k})}}2

If all the atoms are identical, then Equation (1) becomesI(q)=f2j=1Nk=1Neiq(RjRk){\displaystyle I(\mathbf {q} )=f^{2}\sum _{j=1}^{N}\sum _{k=1}^{N}\mathrm {e} ^{-i\mathbf {q} \cdot (\mathbf {R} _{j}-\mathbf {R} _{k})}} andj=1Nfj2=Nf2{\displaystyle \sum _{j=1}^{N}f_{j}^{2}=Nf^{2}} so

S(q)=1Nj=1Nk=1Neiq(RjRk){\displaystyle S(\mathbf {q} )={\frac {1}{N}}\sum _{j=1}^{N}\sum _{k=1}^{N}\mathrm {e} ^{-i\mathbf {q} \cdot (\mathbf {R} _{j}-\mathbf {R} _{k})}}3

Another useful simplification is if the material is isotropic, like a powder or a simple liquid. In that case, the intensity depends onq=|q|{\displaystyle q=|\mathbf {q} |} andrjk=|rjrk|{\displaystyle r_{jk}=|\mathbf {r} _{j}-\mathbf {r} _{k}|}. In three dimensions, Equation (2) then simplifies to the Debye scattering equation:[1]

S(q)=1j=1Nfj2j=1Nk=1Nfjfksin(qrjk)qrjk{\displaystyle S(\mathbf {q} )={\frac {1}{\sum _{j=1}^{N}f_{j}^{2}}}\sum _{j=1}^{N}\sum _{k=1}^{N}f_{j}f_{k}{\frac {\sin(qr_{jk})}{qr_{jk}}}}4

An alternative derivation gives good insight, but usesFourier transforms andconvolution. To be general, consider a scalar (real) quantityϕ(r){\displaystyle \phi (\mathbf {r} )} defined in a volumeV{\displaystyle V}; this may correspond, for instance, to a mass or charge distribution or to the refractive index of an inhomogeneous medium. If the scalar function is integrable, we can write itsFourier transform asψ(q)=Vϕ(r)exp(iqr)dr{\displaystyle \textstyle \psi (\mathbf {q} )=\int _{V}\phi (\mathbf {r} )\exp(-i\mathbf {q} \cdot \mathbf {r} )\,\mathrm {d} \mathbf {r} }. In theBorn approximation the amplitude of the scattered wave corresponding to the scattering vectorq{\displaystyle \mathbf {q} } is proportional to the Fourier transformψ(q){\displaystyle \textstyle \psi (\mathbf {q} )}.[1] When the system under study is composed of a numberN{\displaystyle N} of identical constituents (atoms, molecules, colloidal particles, etc.) each of which has a distribution of mass or chargef(r){\displaystyle f(\mathbf {r} )} then the total distribution can be considered the convolution of this function with a set ofdelta functions.

ϕ(r)=j=1Nf(rRj)=f(r)j=1Nδ(rRj),{\displaystyle \phi (\mathbf {r} )=\sum _{j=1}^{N}f(\mathbf {r} -\mathbf {R} _{j})=f(\mathbf {r} )\ast \sum _{j=1}^{N}\delta (\mathbf {r} -\mathbf {R} _{j}),}5

withRj,j=1,,N{\displaystyle \textstyle \mathbf {R} _{j},j=1,\,\ldots ,\,N} the particle positions as before. Using the property that the Fourier transform of a convolution product is simply the product of the Fourier transforms of the two factors, we haveψ(q)=f(q)×j=1Nexp(iqRj){\displaystyle \textstyle \psi (\mathbf {q} )=f(\mathbf {q} )\times \sum _{j=1}^{N}\exp(-i\mathbf {q} \cdot \mathbf {R} _{j})}, so that:

I(q)=|f(q)|2×(j=1NeiqRj)×(k=1NeiqRk)=|f(q)|2j=1Nk=1Neiq(RjRk).{\displaystyle I(\mathbf {q} )=\left|f(\mathbf {q} )\right|^{2}\times \left(\sum _{j=1}^{N}\mathrm {e} ^{-i\mathbf {q} \cdot \mathbf {R} _{j}}\right)\times \left(\sum _{k=1}^{N}\mathrm {e} ^{i\mathbf {q} \cdot \mathbf {R} _{k}}\right)=\left|f(\mathbf {q} )\right|^{2}\sum _{j=1}^{N}\sum _{k=1}^{N}\mathrm {e} ^{-i\mathbf {q} \cdot (\mathbf {R} _{j}-\mathbf {R} _{k})}.}6

This is clearly the same as Equation (1) with all particles identical, except that heref{\displaystyle f} is shown explicitly as a function ofq{\displaystyle \mathbf {q} }.

In general, the particle positions are not fixed and the measurement takes place over a finite exposure time and with a macroscopic sample (much larger than the interparticle distance). The experimentally accessible intensity is thus an averaged oneI(q){\displaystyle \textstyle \langle I(\mathbf {q} )\rangle }; we need not specify whether{\displaystyle \langle \cdot \rangle } denotes a time orensemble average. To take this into account we can rewrite Equation (3) as:

S(q)=1Nj=1Nk=1Neiq(RjRk).{\displaystyle S(\mathbf {q} )={\frac {1}{N}}\left\langle \sum _{j=1}^{N}\sum _{k=1}^{N}\mathrm {e} ^{-i\mathbf {q} \cdot (\mathbf {R} _{j}-\mathbf {R} _{k})}\right\rangle .}7

Perfect crystals

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In acrystal, the constitutive particles are arranged periodically, withtranslational symmetry forming alattice. The crystal structure can be described as aBravais lattice with a group of atoms, called the basis, placed at every lattice point; that is, [crystal structure] = [lattice]{\displaystyle \ast } [basis]. If the lattice is infinite and completely regular, the system is aperfect crystal. For such a system, only a set of specific values forq{\displaystyle \mathbf {q} } can give scattering, and the scattering amplitude for all other values is zero. This set of values forms a lattice, called thereciprocal lattice, which is the Fourier transform of the real-space crystal lattice.

In principle the scattering factorS(q){\displaystyle S(\mathbf {q} )} can be used to determine the scattering from a perfect crystal; in the simple case when the basis is a single atom at the origin (and again neglecting all thermal motion, so that there is no need for averaging) all the atoms have identical environments. Equation (1) can be written as

I(q)=f2|j=1NeiqRj|2{\displaystyle I(\mathbf {q} )=f^{2}\left|\sum _{j=1}^{N}\mathrm {e} ^{-i\mathbf {q} \cdot \mathbf {R} _{j}}\right|^{2}} andS(q)=1N|j=1NeiqRj|2{\displaystyle S(\mathbf {q} )={\frac {1}{N}}\left|\sum _{j=1}^{N}\mathrm {e} ^{-i\mathbf {q} \cdot \mathbf {R} _{j}}\right|^{2}}.

The structure factor is then simply the squared modulus of theFourier transform of the lattice, and shows the directions in which scattering can have non-zero intensity. At these values ofq{\displaystyle \mathbf {q} } the wave from every lattice point is in phase. The value of the structure factor is the same for all these reciprocal lattice points, and the intensity varies only due to changes inf{\displaystyle f} withq{\displaystyle \mathbf {q} }.

Units

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The units of the structure-factor amplitude depend on the incident radiation. For X-ray crystallography they are multiples of the unit of scattering by a single electron (2.82×1015{\displaystyle \times 10^{-15}} m); for neutron scattering by atomic nuclei the unit of scattering length of1014{\displaystyle 10^{-14}} m is commonly used.

The above discussion uses the wave vectors|k|=2π/λ{\displaystyle |\mathbf {k} |=2\pi /\lambda } and|q|=4πsinθ/λ{\displaystyle |\mathbf {q} |=4\pi \sin \theta /\lambda }. However, crystallography often uses wave vectors|s|=1/λ{\displaystyle |\mathbf {s} |=1/\lambda } and|g|=2sinθ/λ{\displaystyle |\mathbf {g} |=2\sin \theta /\lambda }. Therefore, when comparing equations from different sources, the factor2π{\displaystyle 2\pi } may appear and disappear, and care to maintain consistent quantities is required to get correct numerical results.

Definition ofFhkl

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In crystallography, the basis and lattice are treated separately. For a perfect crystal the lattice gives thereciprocal lattice, which determines the positions (angles) of diffracted beams, and the basis gives the structure factorFhkl{\displaystyle F_{hkl}} which determines the amplitude and phase of the diffracted beams:

Fhk=j=1Nfje[2πi(hxj+kyj+zj)],{\displaystyle F_{hk\ell }=\sum _{j=1}^{N}f_{j}\mathrm {e} ^{[-2\pi i(hx_{j}+ky_{j}+\ell z_{j})]},}8

where the sum is over all atoms in the unit cell,xj,yj,zj{\displaystyle x_{j},y_{j},z_{j}} are the positional coordinates of thej{\displaystyle j}-th atom, andfj{\displaystyle f_{j}} is the scattering factor of thej{\displaystyle j}-th atom.[4] The coordinatesxj,yj,zj{\displaystyle x_{j},y_{j},z_{j}} have the directions and dimensions of the lattice vectorsa,b,c{\displaystyle \mathbf {a} ,\mathbf {b} ,\mathbf {c} }. That is, (0,0,0) is at the lattice point, the origin of position in the unit cell; (1,0,0) is at the next lattice point alonga{\displaystyle \mathbf {a} } and (1/2, 1/2, 1/2) is at the body center of the unit cell.(hkl){\displaystyle (hkl)} defines areciprocal lattice point at(ha,kb,lc){\displaystyle (h\mathbf {a^{*}} ,k\mathbf {b^{*}} ,l\mathbf {c^{*}} )} which corresponds to the real-space plane defined by theMiller indices(hkl){\displaystyle (hkl)} (seeBragg's law).

Fhk{\displaystyle F_{hk\ell }} is the vector sum of waves from all atoms within the unit cell. An atom at any lattice point has the reference phase angle zero for allhk{\displaystyle hk\ell } since then(hxj+kyj+zj){\displaystyle (hx_{j}+ky_{j}+\ell z_{j})} is always an integer. A wave scattered from an atom at (1/2, 0, 0) will be in phase ifh{\displaystyle h} is even, out of phase ifh{\displaystyle h} is odd.

Again an alternative view using convolution can be helpful. Since [crystal structure] = [lattice]{\displaystyle \ast } [basis],F{\displaystyle {\mathcal {F}}}[crystal structure] =F{\displaystyle {\mathcal {F}}}[lattice]×F{\displaystyle \times {\mathcal {F}}}[basis]; that is, scattering{\displaystyle \propto } [reciprocal lattice]×{\displaystyle \times } [structure factor].

Examples ofFhkl in 3-D

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Body-centered cubic (BCC)

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For the body-centered cubic Bravais lattice (cI), we use the points(0,0,0){\displaystyle (0,0,0)} and(12,12,12){\displaystyle ({\tfrac {1}{2}},{\tfrac {1}{2}},{\tfrac {1}{2}})} which leads us to

Fhk=jfje2πi(hxj+kyj+zj)=f[1+(eiπ)h+k+]=f[1+(1)h+k+]{\displaystyle F_{hk\ell }=\sum _{j}f_{j}e^{-2\pi i(hx_{j}+ky_{j}+\ell z_{j})}=f\left[1+\left(e^{-i\pi }\right)^{h+k+\ell }\right]=f\left[1+(-1)^{h+k+\ell }\right]}

and hence

Fhk={2f,h+k+=even0,h+k+=odd{\displaystyle F_{hk\ell }={\begin{cases}2f,&h+k+\ell ={\text{even}}\\0,&h+k+\ell ={\text{odd}}\end{cases}}}

Face-centered cubic (FCC)

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TheFCC lattice is a Bravais lattice, and its Fourier transform is a body-centered cubic lattice. However to obtainFhk{\displaystyle F_{hk\ell }} without this shortcut, consider an FCC crystal with one atom at each lattice point as a primitive or simple cubic with a basis of 4 atoms, at the originxj,yj,zj=(0,0,0){\displaystyle x_{j},y_{j},z_{j}=(0,0,0)} and at the three adjacent face centers,xj,yj,zj=(12,12,0){\displaystyle x_{j},y_{j},z_{j}=\left({\frac {1}{2}},{\frac {1}{2}},0\right)},(0,12,12){\displaystyle \left(0,{\frac {1}{2}},{\frac {1}{2}}\right)} and(12,0,12){\displaystyle \left({\frac {1}{2}},0,{\frac {1}{2}}\right)}. Equation (8) becomes

Fhk=fj=14e[2πi(hxj+kyj+zj)]=f[1+e[iπ(h+k)]+e[iπ(k+)]+e[iπ(h+)]]=f[1+(1)h+k+(1)k++(1)h+]{\displaystyle F_{hk\ell }=f\sum _{j=1}^{4}\mathrm {e} ^{[-2\pi i(hx_{j}+ky_{j}+\ell z_{j})]}=f\left[1+\mathrm {e} ^{[-i\pi (h+k)]}+\mathrm {e} ^{[-i\pi (k+\ell )]}+\mathrm {e} ^{[-i\pi (h+\ell )]}\right]=f\left[1+(-1)^{h+k}+(-1)^{k+\ell }+(-1)^{h+\ell }\right]}

with the result

Fhk={4f,h,k,  all even or all odd0,h,k,  mixed parity{\displaystyle F_{hk\ell }={\begin{cases}4f,&h,k,\ell \ \ {\mbox{all even or all odd}}\\0,&h,k,\ell \ \ {\mbox{mixed parity}}\end{cases}}}

The most intense diffraction peak from a material that crystallizes in the FCC structure is typically the (111). Films of FCC materials likegold tend to grow in a (111) orientation with a triangular surface symmetry. A zero diffracted intensity for a group of diffracted beams (here,h,k,{\displaystyle h,k,\ell } of mixed parity) is called a systematic absence.

Diamond crystal structure

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Thediamond cubic crystal structure occurs for examplediamond (carbon),tin, and mostsemiconductors. There are 8 atoms in the cubic unit cell. We can consider the structure as a simple cubic with a basis of 8 atoms, at positions

xj,yj,zj=(0, 0, 0)(12, 12, 0) (0, 12, 12)(12, 0, 12)(14, 14, 14)(34, 34, 14) (14, 34, 34)(34, 14, 34){\displaystyle {\begin{aligned}x_{j},y_{j},z_{j}=&(0,\ 0,\ 0)&\left({\frac {1}{2}},\ {\frac {1}{2}},\ 0\right)\ &\left(0,\ {\frac {1}{2}},\ {\frac {1}{2}}\right)&\left({\frac {1}{2}},\ 0,\ {\frac {1}{2}}\right)\\&\left({\frac {1}{4}},\ {\frac {1}{4}},\ {\frac {1}{4}}\right)&\left({\frac {3}{4}},\ {\frac {3}{4}},\ {\frac {1}{4}}\right)\ &\left({\frac {1}{4}},\ {\frac {3}{4}},\ {\frac {3}{4}}\right)&\left({\frac {3}{4}},\ {\frac {1}{4}},\ {\frac {3}{4}}\right)\\\end{aligned}}}

But comparing this to the FCC above, we see that it is simpler to describe the structure as FCC with a basis of two atoms at (0, 0, 0) and (1/4, 1/4, 1/4). For this basis, Equation (8) becomes:

Fhk(basis)=fj=12e[2πi(hxj+kyj+zj)]=f[1+e[iπ/2(h+k+)]]=f[1+(i)h+k+]{\displaystyle F_{hk\ell }({\rm {{basis})=f\sum _{j=1}^{2}\mathrm {e} ^{[-2\pi i(hx_{j}+ky_{j}+\ell z_{j})]}=f\left[1+\mathrm {e} ^{[-i\pi /2(h+k+\ell )]}\right]=f\left[1+(-i)^{h+k+\ell }\right]}}}

And then the structure factor for the diamond cubic structure is the product of this and the structure factor for FCC above, (only including the atomic form factor once)

Fhk=f[1+(1)h+k+(1)k++(1)h+]×[1+(i)h+k+]{\displaystyle F_{hk\ell }=f\left[1+(-1)^{h+k}+(-1)^{k+\ell }+(-1)^{h+\ell }\right]\times \left[1+(-i)^{h+k+\ell }\right]}

with the result

These points are encapsulated by the following equations:

Fhk={8f,h+k+=4N4(1±i)f,h+k+=2N+10,h+k+=4N+2{\displaystyle F_{hk\ell }={\begin{cases}8f,&h+k+\ell =4N\\4(1\pm i)f,&h+k+\ell =2N+1\\0,&h+k+\ell =4N+2\\\end{cases}}}
|Fhk|2={64f2,h+k+=4N32f2,h+k+=2N+10,h+k+=4N+2{\displaystyle \Rightarrow |F_{hk\ell }|^{2}={\begin{cases}64f^{2},&h+k+\ell =4N\\32f^{2},&h+k+\ell =2N+1\\0,&h+k+\ell =4N+2\\\end{cases}}}

whereN{\displaystyle N} is an integer.

Zincblende crystal structure

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The zincblende structure is similar to the diamond structure except that it is a compound of two distinct interpenetrating fcc lattices, rather than all the same element. Denoting the two elements in the compound byA{\displaystyle A} andB{\displaystyle B}, the resulting structure factor is

Fhk={4(fA+fB),h+k+=4N4(fA±ifB),h+k+=2N+14(fAfB),h+k+=4N+2{\displaystyle F_{hk\ell }={\begin{cases}4(f_{A}+f_{B}),&h+k+\ell =4N\\4(f_{A}\pm if_{B}),&h+k+\ell =2N+1\\4(f_{A}-f_{B}),&h+k+\ell =4N+2\\\end{cases}}}

Cesium chloride

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Cesium chloride is a simple cubic crystal lattice with a basis of Cs at (0,0,0) and Cl at (1/2, 1/2, 1/2) (or the other way around, it makes no difference). Equation (8) becomes

Fhk=j=12fje[2πi(hxj+kyj+zj)]=[fCs+fCle[iπ(h+k+)]]=[fCs+fCl(1)h+k+]{\displaystyle F_{hk\ell }=\sum _{j=1}^{2}f_{j}\mathrm {e} ^{[-2\pi i(hx_{j}+ky_{j}+\ell z_{j})]}=\left[f_{Cs}+f_{Cl}\mathrm {e} ^{[-i\pi (h+k+\ell )]}\right]=\left[f_{Cs}+f_{Cl}(-1)^{h+k+\ell }\right]}

We then arrive at the following result for the structure factor for scattering from a plane(hk){\displaystyle (hk\ell )}:

Fhk={(fCs+fCl),h+k+even(fCsfCl),h+k+odd{\displaystyle F_{hk\ell }={\begin{cases}(f_{Cs}+f_{Cl}),&h+k+\ell &{\text{even}}\\(f_{Cs}-f_{Cl}),&h+k+\ell &{\text{odd}}\end{cases}}}

and for scattered intensity,|Fhk|2={(fCs+fCl)2,h+k+even(fCsfCl)2,h+k+odd{\displaystyle |F_{hk\ell }|^{2}={\begin{cases}(f_{Cs}+f_{Cl})^{2},&h+k+\ell &{\text{even}}\\(f_{Cs}-f_{Cl})^{2},&h+k+\ell &{\text{odd}}\end{cases}}}

Hexagonal close-packed (HCP)

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In an HCP crystal such asgraphite, the two coordinates include the origin(0,0,0){\displaystyle \left(0,0,0\right)} and the next plane up thec axis located atc/2, and hence(1/3,2/3,1/2){\displaystyle \left(1/3,2/3,1/2\right)}, which gives us

Fhk=f[1+e2πi(h3+2k3+2)]{\displaystyle F_{hk\ell }=f\left[1+e^{2\pi i\left({\tfrac {h}{3}}+{\tfrac {2k}{3}}+{\tfrac {\ell }{2}}\right)}\right]}

From this it is convenient to define dummy variableXh/3+2k/3+/2{\displaystyle X\equiv h/3+2k/3+\ell /2}, and from there consider the modulus squared so hence

|F|2=f2(1+e2πiX)(1+e2πiX)=f2(2+e2πiX+e2πiX)=f2(2+2cos[2πX])=f2(4cos2[πX]){\displaystyle |F|^{2}=f^{2}\left(1+e^{2\pi iX}\right)\left(1+e^{-2\pi iX}\right)=f^{2}\left(2+e^{2\pi iX}+e^{-2\pi iX}\right)=f^{2}\left(2+2\cos[2\pi X]\right)=f^{2}\left(4\cos ^{2}\left[\pi X\right]\right)}

This leads us to the following conditions for the structure factor:

|Fhk|2={0,h+2k=3N and  is odd,4f2,h+2k=3N and  is even,3f2,h+2k=3N±1 and  is odd,f2,h+2k=3N±1 and  is even{\displaystyle |F_{hk\ell }|^{2}={\begin{cases}0,&h+2k=3N{\text{ and }}\ell {\text{ is odd,}}\\4f^{2},&h+2k=3N{\text{ and }}\ell {\text{ is even,}}\\3f^{2},&h+2k=3N\pm 1{\text{ and }}\ell {\text{ is odd,}}\\f^{2},&h+2k=3N\pm 1{\text{ and }}\ell {\text{ is even}}\\\end{cases}}}

Perfect crystals in one and two dimensions

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The reciprocal lattice is easily constructed in one dimension: for particles on a line with a perioda{\displaystyle a}, the reciprocal lattice is an infinite array of points with spacing2π/a{\displaystyle 2\pi /a}. In two dimensions, there are only fiveBravais lattices. The corresponding reciprocal lattices have the same symmetry as the direct lattice. 2-D lattices are excellent for demonstrating simple diffraction geometry on a flat screen, as below. Equations (1)–(7) for structure factorS(q){\displaystyle S(\mathbf {q} )} apply with a scattering vector of limited dimensionality and a crystallographic structure factor can be defined in 2-D asFhk=j=1Nfje[2πi(hxj+kyj)]{\displaystyle F_{hk}=\sum _{j=1}^{N}f_{j}\mathrm {e} ^{[-2\pi i(hx_{j}+ky_{j})]}}.

However, recall that real 2-D crystals such asgraphene exist in 3-D. The reciprocal lattice of a 2-D hexagonal sheet that exists in 3-D space in thexy{\displaystyle xy} plane is a hexagonal array of lines parallel to thez{\displaystyle z} orz{\displaystyle z^{*}} axis that extend to±{\displaystyle \pm \infty } and intersect any plane of constantz{\displaystyle z} in a hexagonal array of points.

Diagram of scattering by a square (planar) lattice. The incident and outgoing beam are shown, as well as the relation between their wave vectorski{\displaystyle \mathbf {k} _{i}},ko{\displaystyle \mathbf {k} _{o}} and the scattering vectorq{\displaystyle \mathbf {q} }.

The Figure shows the construction of one vector of a 2-D reciprocal lattice and its relation to a scattering experiment.

A parallel beam, with wave vectorki{\displaystyle \mathbf {k} _{i}} is incident on a square lattice of parametera{\displaystyle a}. The scattered wave is detected at a certain angle, which defines the wave vector of the outgoing beam,ko{\displaystyle \mathbf {k} _{o}} (under the assumption ofelastic scattering,|ko|=|ki|{\displaystyle |\mathbf {k} _{o}|=|\mathbf {k} _{i}|}). One can equally define the scattering vectorq=koki{\displaystyle \mathbf {q} =\mathbf {k} _{o}-\mathbf {k} _{i}} and construct the harmonic patternexp(iqr){\displaystyle \exp(i\mathbf {q} \mathbf {r} )}. In the depicted example, the spacing of this pattern coincides to the distance between particle rows:q=2π/a{\displaystyle q=2\pi /a}, so that contributions to the scattering from all particles are in phase (constructive interference). Thus, the total signal in directionko{\displaystyle \mathbf {k} _{o}} is strong, andq{\displaystyle \mathbf {q} } belongs to the reciprocal lattice. It is easily shown that this configuration fulfillsBragg's law.

Structure factor of a periodic chain, for different particle numbersN{\displaystyle N}.

Imperfect crystals

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Technically a perfect crystal must be infinite, so a finite size is an imperfection. Real crystals always exhibit imperfections of their order besides their finite size, and these imperfections can have profound effects on the properties of the material.André Guinier[5] proposed a widely employed distinction between imperfections that preserve thelong-range order of the crystal that he calleddisorder of the first kind and those that destroy it calleddisorder of the second kind. An example of the first is thermal vibration; an example of the second is some density of dislocations.

The generally applicable structure factorS(q){\displaystyle S(\mathbf {q} )} can be used to include the effect of any imperfection. In crystallography, these effects are treated as separate from the structure factorFhkl{\displaystyle F_{hkl}}, so separate factors for size or thermal effects are introduced into the expressions for scattered intensity, leaving the perfect crystal structure factor unchanged. Therefore, a detailed description of these factors in crystallographic structure modeling and structure determination by diffraction is not appropriate in this article.

Finite-size effects

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ForS(q){\displaystyle S(q)} a finite crystal means that the sums in equations 1-7 are now over a finiteN{\displaystyle N}. The effect is most easily demonstrated with a 1-D lattice of points. The sum of the phase factors is a geometric series and the structure factor becomes:

S(q)=1N|1eiNqa1eiqa|2=1N[sin(Nqa/2)sin(qa/2)]2.{\displaystyle S(q)={\frac {1}{N}}\left|{\frac {1-\mathrm {e} ^{-iNqa}}{1-\mathrm {e} ^{-iqa}}}\right|^{2}={\frac {1}{N}}\left[{\frac {\sin(Nqa/2)}{\sin(qa/2)}}\right]^{2}.}

This function is shown in the Figure for different values ofN{\displaystyle N}.When the scattering from every particle is in phase, which is when the scattering is at a reciprocal lattice pointq=2kπ/a{\displaystyle q=2k\pi /a}, the sum of the amplitudes must beN{\displaystyle \propto N} and so the maxima in intensity areN2{\displaystyle \propto N^{2}}. Taking the above expression forS(q){\displaystyle S(q)} and estimating the limitS(q0){\displaystyle S(q\to 0)} using, for instance,L'Hôpital's rule) shows thatS(q=2kπ/a)=N{\displaystyle S(q=2k\pi /a)=N} as seen in the Figure. At the midpointS(q=(2k+1)π/a)=1/N{\displaystyle S(q=(2k+1)\pi /a)=1/N} (by direct evaluation) and the peak width decreases like1/N{\displaystyle 1/N}. In the largeN{\displaystyle N} limit, the peaks become infinitely sharp Dirac delta functions, the reciprocal lattice of the perfect 1-D lattice.

In crystallography whenFhkl{\displaystyle F_{hkl}} is used,N{\displaystyle N} is large, and the formal size effect on diffraction is taken as[sin(Nqa/2)(qa/2)]2{\displaystyle \left[{\frac {\sin(Nqa/2)}{(qa/2)}}\right]^{2}}, which is the same as the expression forS(q){\displaystyle S(q)} above near to the reciprocal lattice points,q2kπ/a{\displaystyle q\approx 2k\pi /a}. Using convolution, we can describe the finite real crystal structure as [lattice]{\displaystyle \ast } [basis]×{\displaystyle \times }rectangular function, where the rectangular function has a value 1 inside the crystal and 0 outside it. ThenF{\displaystyle {\mathcal {F}}}[crystal structure] =F{\displaystyle {\mathcal {F}}}[lattice]×F{\displaystyle \times {\mathcal {F}}}[basis]F{\displaystyle \ast {F}}[rectangular function]; that is, scattering{\displaystyle \propto } [reciprocal lattice]×{\displaystyle \times } [structure factor]{\displaystyle \ast } [sinc function]. Thus the intensity, which is a delta function of position for the perfect crystal, becomes asinc2{\textstyle \operatorname {sinc} ^{2}} function around every point with a maximumN2{\displaystyle \propto N^{2}}, a width1/N{\displaystyle \propto 1/N}, areaN{\displaystyle \propto N}.

Disorder of the first kind

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This model for disorder in a crystal starts with the structure factor of a perfect crystal. In one-dimension for simplicity and withN planes, we then start with the expression above for a perfect finite lattice, and then this disorder only changesS(q){\displaystyle S(q)} by a multiplicative factor, to give[1]

S(q)=1N[sin(Nqa/2)sin(qa/2)]2exp(q2δx2){\displaystyle S(q)={\frac {1}{N}}\left[{\frac {\sin(Nqa/2)}{\sin(qa/2)}}\right]^{2}\exp \left(-q^{2}\langle \delta x^{2}\rangle \right)}

where the disorder is measured by the mean-square displacement of the positionsxj{\displaystyle x_{j}} from their positions in a perfect one-dimensional lattice:a(j(N1)/2){\displaystyle a(j-(N-1)/2)}, i.e.,xj=a(j(N1)/2)+δx{\displaystyle x_{j}=a(j-(N-1)/2)+\delta x}, whereδx{\displaystyle \delta x} is a small (much less thana{\displaystyle a}) random displacement. For disorder of the first kind, each random displacementδx{\displaystyle \delta x} is independent of the others, and with respect to a perfect lattice. Thus the displacementsδx{\displaystyle \delta x} do not destroy the translational order of the crystal. This has the consequence that for infinite crystals (N{\displaystyle N\to \infty }) the structure factor still has delta-function Bragg peaks – the peak width still goes to zero asN{\displaystyle N\to \infty }, with this kind of disorder. However, it does reduce the amplitude of the peaks, and due to the factor ofq2{\displaystyle q^{2}} in the exponential factor, it reduces peaks at largeq{\displaystyle q} much more than peaks at smallq{\displaystyle q}.

The structure is simply reduced by aq{\displaystyle q} and disorder dependent term because all disorder of the first-kind does is smear out the scattering planes, effectively reducing the form factor.

In three dimensions the effect is the same, the structure is again reduced by a multiplicative factor, and this factor is often called theDebye–Waller factor. Note that the Debye–Waller factor is often ascribed to thermal motion, i.e., theδx{\displaystyle \delta x} are due to thermal motion, but any random displacements about a perfect lattice, not just thermal ones, will contribute to the Debye–Waller factor.

Disorder of the second kind

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However, fluctuations that cause the correlations between pairs of atoms to decrease as their separation increases, causes the Bragg peaks in the structure factor of a crystal to broaden. To see how this works, we consider a one-dimensional toy model: a stack of plates with mean spacinga{\displaystyle a}. The derivation follows that in chapter 9 of Guinier's textbook.[6] This model has been pioneered by and applied to a number of materials by Hosemann and collaborators[7] over a number of years. Guinier and they termed this disorder of the second kind, and Hosemann in particular referred to this imperfect crystalline ordering asparacrystalline ordering. Disorder of the first kind is the source of theDebye–Waller factor.

To derive the model we start with the definition (in one dimension) of the

S(q)=1Nj,k=1Neiq(xjxk){\displaystyle S(q)={\frac {1}{N}}\sum _{j,k=1}^{N}\mathrm {e} ^{-iq(x_{j}-x_{k})}}

To start with we will consider, for simplicity an infinite crystal, i.e.,N{\displaystyle N\to \infty }. We will consider a finite crystal with disorder of the second-type below.

For our infinite crystal, we want to consider pairs of lattice sites. For large each plane of an infinite crystal, there are two neighboursm{\displaystyle m} planes away, so the above double sum becomes a single sum over pairs of neighbours either side of an atom, at positionsm{\displaystyle -m} andm{\displaystyle m} lattice spacings away, timesN{\displaystyle N}. So, then

S(q)=1+2m=1d(Δx)pm(Δx)cos(qΔx){\displaystyle S(q)=1+2\sum _{m=1}^{\infty }\int _{-\infty }^{\infty }{\rm {d}}(\Delta x)p_{m}(\Delta x)\cos \left(q\Delta x\right)}

wherepm(Δx){\displaystyle p_{m}(\Delta x)} is the probability density function for the separationΔx{\displaystyle \Delta x} of a pair of planes,m{\displaystyle m} lattice spacings apart. For the separation of neighbouring planes we assume for simplicity that the fluctuations around the mean neighbour spacing ofa are Gaussian, i.e., that

p1(Δx)=1(2πσ22)1/2exp[(Δxa)2/(2σ22)]{\displaystyle p_{1}(\Delta x)={\frac {1}{\left(2\pi \sigma _{2}^{2}\right)^{1/2}}}\exp \left[-\left(\Delta x-a\right)^{2}/(2\sigma _{2}^{2})\right]}

and we also assume that the fluctuations between a plane and its neighbour, and between this neighbour and the next plane, are independent. Thenp2(Δx){\displaystyle p_{2}(\Delta x)} is just the convolution of twop1(Δx){\displaystyle p_{1}(\Delta x)}s, etc. As the convolution of two Gaussians is just another Gaussian, we have that

pm(Δx)=1(2πmσ22)1/2exp[(Δxma)2/(2mσ22)]{\displaystyle p_{m}(\Delta x)={\frac {1}{\left(2\pi m\sigma _{2}^{2}\right)^{1/2}}}\exp \left[-\left(\Delta x-ma\right)^{2}/(2m\sigma _{2}^{2})\right]}

The sum inS(q){\displaystyle S(q)} is then just a sum of Fourier transforms of Gaussians, and so

S(q)=1+2m=1rmcos(mqa){\displaystyle S(q)=1+2\sum _{m=1}^{\infty }r^{m}\cos \left(mqa\right)}

forr=exp[q2σ22/2]{\displaystyle r=\exp[-q^{2}\sigma _{2}^{2}/2]}. The sum is just the real part of the summ=1[rexp(iqa)]m{\displaystyle \sum _{m=1}^{\infty }[r\exp(iqa)]^{m}} and so the structure factor of the infinite but disordered crystal is

S(q)=1r21+r22rcos(qa){\displaystyle S(q)={\frac {1-r^{2}}{1+r^{2}-2r\cos(qa)}}}

This has peaks at maximaqp=2nπ/a{\displaystyle q_{p}=2n\pi /a}, wherecos(qPa)=1{\displaystyle \cos(q_{P}a)=1}. These peaks have heights

S(qP)=1+r1r4qP2σ22=a2n2π2σ22{\displaystyle S(q_{P})={\frac {1+r}{1-r}}\approx {\frac {4}{q_{P}^{2}\sigma _{2}^{2}}}={\frac {a^{2}}{n^{2}\pi ^{2}\sigma _{2}^{2}}}}

i.e., the height of successive peaks drop off as the order of the peak (and soq{\displaystyle q}) squared. Unlike finite-size effects that broaden peaks but do not decrease their height, disorder lowers peak heights. Note that here we assuming that the disorder is relatively weak, so that we still have relatively well defined peaks. This is the limitqσ21{\displaystyle q\sigma _{2}\ll 1}, wherer1q2σ22/2{\displaystyle r\simeq 1-q^{2}\sigma _{2}^{2}/2}. In this limit, near a peak we can approximatecos(qa)1(Δq)2a2/2{\displaystyle \cos(qa)\simeq 1-(\Delta q)^{2}a^{2}/2}, withΔq=qqP{\displaystyle \Delta q=q-q_{P}} and obtain

S(q)S(qP)1+r(1r)2Δq2a22S(qP)1+Δq2[qP2σ22/a]2/2{\displaystyle S(q)\approx {\frac {S(q_{P})}{1+{\frac {r}{(1-r)^{2}}}{\frac {\Delta q^{2}a^{2}}{2}}}}\approx {\frac {S(q_{P})}{1+{\frac {\Delta q^{2}}{[q_{P}^{2}\sigma _{2}^{2}/a]^{2}/2}}}}}

which is aLorentzian or Cauchy function, of FWHMqP2σ22/a=4π2n2(σ2/a)2/a{\displaystyle q_{P}^{2}\sigma _{2}^{2}/a=4\pi ^{2}n^{2}(\sigma _{2}/a)^{2}/a}, i.e., the FWHM increases as the square of the order of peak, and so as the square of the wave vectorq{\displaystyle q} at the peak.

Finally, the product of the peak height and the FWHM is constant and equals4/a{\displaystyle 4/a}, in theqσ21{\displaystyle q\sigma _{2}\ll 1} limit. For the first few peaks wheren{\displaystyle n} is not large, this is just theσ2/a1{\displaystyle \sigma _{2}/a\ll 1} limit.

Finite crystals with disorder of the second kind

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For a one-dimensional crystal of sizeN{\displaystyle N}

S(q)=1+2m=1N(1mN)rmcos(mqa){\displaystyle S(q)=1+2\sum _{m=1}^{N}\left(1-{\frac {m}{N}}\right)r^{m}\cos \left(mqa\right)}

where the factor in parentheses comes from the fact the sum is over nearest-neighbour pairs (m=1{\displaystyle m=1}), next nearest-neighbours (m=2{\displaystyle m=2}), ... and for a crystal ofN{\displaystyle N} planes, there areN1{\displaystyle N-1} pairs of nearest neighbours,N2{\displaystyle N-2} pairs of next-nearest neighbours, etc.

Liquids

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In contrast with crystals, liquids have nolong-range order (in particular, there is no regular lattice), so the structure factor does not exhibit sharp peaks. They do however show a certain degree ofshort-range order, depending on their density and on the strength of the interaction between particles. Liquids are isotropic, so that, after the averaging operation in Equation (4), the structure factor only depends on the absolute magnitude of the scattering vectorq=|q|{\displaystyle q=\left|\mathbf {q} \right|}. For further evaluation, it is convenient to separate the diagonal termsj=k{\displaystyle j=k} in the double sum, whose phase is identically zero, and therefore each contribute a unit constant:

S(q)=1+1Njkeiq(RjRk){\displaystyle S(q)=1+{\frac {1}{N}}\left\langle \sum _{j\neq k}\mathrm {e} ^{-i\mathbf {q} (\mathbf {R} _{j}-\mathbf {R} _{k})}\right\rangle }.9

One can obtain an alternative expression forS(q){\displaystyle S(q)} in terms of theradial distribution functiong(r){\displaystyle g(r)}:[8]

S(q)=1+ρVdreiqrg(r){\displaystyle S(q)=1+\rho \int _{V}\mathrm {d} \mathbf {r} \,\mathrm {e} ^{-i\mathbf {q} \mathbf {r} }g(r)}.10

Ideal gas

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In the limiting case of no interaction, the system is anideal gas and the structure factor is completely featureless:S(q)=1{\displaystyle S(q)=1}, because there is no correlation between the positionsRj{\displaystyle \mathbf {R} _{j}} andRk{\displaystyle \mathbf {R} _{k}} of different particles (they areindependent random variables), so the off-diagonal terms in Equation (9) average to zero:exp[iq(RjRk)]=exp(iqRj)exp(iqRk)=0{\displaystyle \langle \exp[-i\mathbf {q} (\mathbf {R} _{j}-\mathbf {R} _{k})]\rangle =\langle \exp(-i\mathbf {q} \mathbf {R} _{j})\rangle \langle \exp(i\mathbf {q} \mathbf {R} _{k})\rangle =0}.

High-q limit

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Even for interacting particles, at high scattering vector the structure factor goes to 1. This result follows from Equation (10), sinceS(q)1{\displaystyle S(q)-1} is theFourier transform of the "regular" functiong(r){\displaystyle g(r)} and thus goes to zero for high values of the argumentq{\displaystyle q}. This reasoning does not hold for a perfect crystal, where the distribution function exhibits infinitely sharp peaks.

Low-q limit

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In the low-q{\displaystyle q} limit, as the system is probed over large length scales, the structure factor contains thermodynamic information, being related to theisothermal compressibilityχT{\displaystyle \chi _{T}} of the liquid by thecompressibility equation:

limq0S(q)=ρkBTχT=kBT(ρp){\displaystyle \lim _{q\rightarrow 0}S(q)=\rho \,k_{\mathrm {B} }T\,\chi _{T}=k_{\mathrm {B} }T\left({\frac {\partial \rho }{\partial p}}\right)}.

Hard-sphere liquids

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Structure factor of a hard-sphere fluid, calculated using the Percus-Yevick approximation, for volume fractionsΦ{\displaystyle \Phi } from 1% to 40%.

In thehard sphere model, the particles are described as impenetrable spheres with radiusR{\displaystyle R}; thus, their center-to-center distancer2R{\displaystyle r\geq 2R} and they experience no interaction beyond this distance. Their interaction potential can be written as:

V(r)={for r<2R,0for r2R.{\displaystyle V(r)={\begin{cases}\infty &{\text{for }}r<2R,\\0&{\text{for }}r\geq 2R.\end{cases}}}

This model has an analytical solution[9] in thePercus–Yevick approximation. Although highly simplified, it provides a good description for systems ranging from liquid metals[10] to colloidal suspensions.[11] In an illustration, the structure factor for a hard-sphere fluid is shown in the Figure, for volume fractionsΦ{\displaystyle \Phi } from 1% to 40%.

Polymers

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Inpolymer systems, the general definition (4) holds; the elementary constituents are now themonomers making up the chains. However, the structure factor being a measure of the correlation between particle positions, one can reasonably expect that this correlation will be different for monomers belonging to the same chain or to different chains.

Let us assume that the volumeV{\displaystyle V} containsNc{\displaystyle N_{c}} identical molecules, each composed ofNp{\displaystyle N_{p}} monomers, such thatNcNp=N{\displaystyle N_{c}N_{p}=N} (Np{\displaystyle N_{p}} is also known as thedegree of polymerization). We can rewrite (4) as:

S(q)=1NcNpαβ=1Ncjk=1Npeiq(RαjRβk)=1NcNpα=1Ncjk=1Npeiq(RαjRαk)+1NcNpαβ=1Ncjk=1Npeiq(RαjRβk){\displaystyle S(\mathbf {q} )={\frac {1}{N_{c}N_{p}}}\left\langle \sum _{\alpha \beta =1}^{N_{c}}\sum _{jk=1}^{N_{p}}\mathrm {e} ^{-i\mathbf {q} (\mathbf {R} _{\alpha j}-\mathbf {R} _{\beta k})}\right\rangle ={\frac {1}{N_{c}N_{p}}}\left\langle \sum _{\alpha =1}^{N_{c}}\sum _{jk=1}^{N_{p}}\mathrm {e} ^{-i\mathbf {q} (\mathbf {R} _{\alpha j}-\mathbf {R} _{\alpha k})}\right\rangle +{\frac {1}{N_{c}N_{p}}}\left\langle \sum _{\alpha \neq \beta =1}^{N_{c}}\sum _{jk=1}^{N_{p}}\mathrm {e} ^{-i\mathbf {q} (\mathbf {R} _{\alpha j}-\mathbf {R} _{\beta k})}\right\rangle },11

where indicesα,β{\displaystyle \alpha ,\beta } label the different molecules andj,k{\displaystyle j,k} the different monomers along each molecule. On the right-hand side we separatedintramolecular (α=β{\displaystyle \alpha =\beta }) andintermolecular (αβ{\displaystyle \alpha \neq \beta }) terms. Using the equivalence of the chains, (11) can be simplified:[12]

S(q)=1Npjk=1Npeiq(RjRk)S1(q)+Nc1Npjk=1Npeiq(R1jR2k){\displaystyle S(\mathbf {q} )=\underbrace {{\frac {1}{N_{p}}}\left\langle \sum _{jk=1}^{N_{p}}\mathrm {e} ^{-i\mathbf {q} (\mathbf {R} _{j}-\mathbf {R} _{k})}\right\rangle } _{S_{1}(q)}+{\frac {N_{c}-1}{N_{p}}}\left\langle \sum _{jk=1}^{N_{p}}\mathrm {e} ^{-i\mathbf {q} (\mathbf {R} _{1j}-\mathbf {R} _{2k})}\right\rangle },12

whereS1(q){\displaystyle S_{1}(q)} is the single-chain structure factor.

See also

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Notes

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  1. ^abcdWarren, B. E. (1969).X-ray Diffraction. Addison Wesley.
  2. ^Cowley, J. M. (1992).Electron Diffraction Techniques Vol 1. Oxford Science.ISBN 9780198555582.
  3. ^Egami, T.; Billinge, S. J. L. (2012).Underneath the Bragg Peaks: Structural Analysis of Complex Material (2nd ed.). Elsevier.ISBN 9780080971339.
  4. ^"Structure Factor".Online Dictionary of CRYSTALLOGRAPHY. IUCr. Retrieved15 September 2016.
  5. ^See Guinier, chapters 6-9
  6. ^Guinier, A (1963).X-Ray Diffraction. San Francisco and London: WH Freeman.
  7. ^Lindenmeyer, PH; Hosemann, R (1963)."Application of the Theory of Paracrystals to the Crystal Structure Analysis of Polyacrylonitrile".Journal of Applied Physics.34 (1): 42.Bibcode:1963JAP....34...42L.doi:10.1063/1.1729086. Archived fromthe original on 2016-08-17.
  8. ^See Chandler, section 7.5.
  9. ^Wertheim, M. (1963). "Exact Solution of the Percus-Yevick Integral Equation for Hard Spheres".Physical Review Letters.10 (8):321–323.Bibcode:1963PhRvL..10..321W.doi:10.1103/PhysRevLett.10.321.
  10. ^Ashcroft, N.; Lekner, J. (1966). "Structure and Resistivity of Liquid Metals".Physical Review.145 (1):83–90.Bibcode:1966PhRv..145...83A.doi:10.1103/PhysRev.145.83.
  11. ^Pusey, P. N.; Van Megen, W. (1986). "Phase behaviour of concentrated suspensions of nearly hard colloidal spheres".Nature.320 (6060): 340.Bibcode:1986Natur.320..340P.doi:10.1038/320340a0.S2CID 4366474.
  12. ^See Teraoka, Section 2.4.4.

References

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  1. Als-Nielsen, N. and McMorrow, D. (2011). Elements of Modern X-ray Physics (2nd edition). John Wiley & Sons.
  2. Guinier, A. (1963). X-ray Diffraction. In Crystals, Imperfect Crystals, and Amorphous Bodies. W. H. Freeman and Co.
  3. Chandler, D. (1987).Introduction to Modern Statistical Mechanics. Oxford University Press.
  4. Hansen, J. P. and McDonald, I. R. (2005). Theory of Simple Liquids (3rd edition). Academic Press.
  5. Teraoka, I. (2002). Polymer Solutions: An Introduction to Physical Properties. John Wiley & Sons.

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