Small-Angle Scattering. Ian W. Hamley

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upper L Baseline left-parenthesis q right-parenthesis 2nd Column equals left pointing angle period right pointing angle left-parenthesis right-parenthesis of sinsin left-parenthesis right-parenthesis times times times 12 qL of coscos phi times times times 12 qL of coscos phi 2 period Subscript phi Baseline equals integral Subscript phi equals 0 Superscript phi equals pi Baseline left-parenthesis StartFraction sine left-parenthesis one half italic q upper L cosine phi right-parenthesis Over one half italic q upper L cosine phi EndFraction right-parenthesis squared sine phi normal d phi 2nd Row 1st Column Blank 2nd Column asymptotically-equals integral Subscript x equals 0 Superscript x equals infinity Baseline left-parenthesis StartFraction sine left-parenthesis one half italic q upper L x right-parenthesis Over one half italic q upper L x EndFraction right-parenthesis squared normal d x equals StartFraction upper L pi Over q EndFraction EndLayout"/>

      The integral over ϕ extends to infinity to make use of the Dirichlet integral, this is valid when q ≥ 2π/L, since the integrand is negligibly small for x > 1 [7]. This leads to the factorization [5, 6]

      The cross‐section intensity is related to the distance distribution function of the cross‐section, γc(r), via the expression [6, 7]

      (1.94)upper I Subscript c Baseline left-parenthesis q right-parenthesis equals 2 pi integral Subscript 0 Superscript upper D Baseline gamma Subscript c Baseline left-parenthesis r right-parenthesis upper J 0 left-parenthesis italic q r right-parenthesis normal d r

      Here D is the cross‐section diameter. For a uniform cylinder this may be evaluated to give [6]

      In these equations J0(qR) and J1(qR) denote Bessel functions of integral order. The cross‐section radius is given by upper R Subscript c Baseline equals upper R slash StartRoot 2 EndRoot [58] (see also the discussion in Section 1.4).

      The pair distribution function of the cross‐section can be obtained from the cross‐section intensity via an inverse Hankel transform [7]

      (1.96)gamma Subscript c Baseline left-parenthesis r right-parenthesis equals StartFraction 1 Over 2 pi EndFraction integral Subscript 0 Superscript infinity Baseline upper I Subscript c Baseline left-parenthesis q right-parenthesis upper J 0 left-parenthesis italic q r right-parenthesis q normal d q

      For flat particles (discs of area A) the intensity can be factored, via an equation analogous to Eq. (1.93) as [4, 6, 10]

      where It(q) is the cross‐section scattering that depends on the thickness T, which is related to the cross‐section radius via upper R Subscript c Baseline equals upper T slash StartRoot 12 EndRoot [58].

      (1.98)upper M Subscript c Baseline equals left-bracket StartFraction normal d sigma Over d upper Omega EndFraction period StartFraction q Over pi EndFraction right-bracket Subscript q right-arrow 0 Baseline period StartFraction upper N Subscript upper A Baseline Over c left-parenthesis upper Delta rho v Subscript p Baseline right-parenthesis squared EndFraction

      where NA is Avogadro's number, vp is the specific volume in cm3 g−1, Δρ is the contrast in cm−2 and q is in cm−1.

      For flat particles, the area per unit length Mt (in g mol−1 cm−2) is obtained from the analogous equation (with q2 dependence cf. Eq. (1.93))

      (1.99)upper M Subscript t Baseline equals left-bracket StartFraction normal d sigma Over d upper Omega EndFraction period StartFraction q squared Over 2 pi EndFraction right-bracket Subscript q right-arrow 0 Baseline period StartFraction upper N Subscript upper A Baseline Over c left-parenthesis upper Delta rho v Subscript p Baseline right-parenthesis squared EndFraction

      The derivations of these equations can be found elsewhere [60].

      Particle polydispersity has a considerable influence on the shape of the form factor. It is included via integration over a particle size distribution D(R′):

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