Past exam of the mathematics course of the University of Cambridge 2010 iii Paper 67 2 Solution Created 2026-10-03 Updated 2026-10-14
Introduce a constant filament bending modulus , which sets the mechanical force scale. The filament has intrinsic curvature of an elastic filament , and its actual signed curvature in a small-slope Monge representation is . To quadratic order one may identify material arc length with in , whileAt fixed positive extension force, the mechanical potential is bending energy minus . Replacing by leaves, up to a force-dependent constant,Its first variation isThe higher-order Euler-Lagrange equation is thereforeFor a Fourier transform relation, take a periodic bulk segment, or a long-filament bulk approximation with negligible endpoint contributions; these are necessary boundary conditions because the question specifies no filament end conditions. Using , every nonzero wavenumber obeysA zero displacement mode is an arbitrary translation. In a periodic representation a constant intrinsic-curvature mode contributes a constant bending cost but no bulk slope, so it does not contribute to the following deficit. The Parseval identity givesFor clarity about finite normalization, on a periodic interval of length define , . Then the equivalent exact quadratic-order formula isThis is force-extension of an intrinsically curved filament, determined by its particular fixed shape rather than by a thermal orientation entropy.
For an ensemble with quenched intrinsic curvature, first minimize each realization and then average the last expression, replacing by its ensemble mean. For stationary bulk disorder, let be the power spectrum, normalized so that its correlation is . The measurable mean deficit per unit projected length isIf the curvature is smooth enough that the second spectral moment is finite, one can take the large-force limit under this integral, obtaining the smooth-curvature high-force extension lawFor a stationary ensemble the integral is . Equivalently, the bulk slope is ; a plot of the mean deficit against measures the mean squared intrinsic-curvature gradient, if is known. The law is a smooth-curvature bulk result, not a universal law for every random filament. For example, ideal white intrinsic-curvature disorder with has an infinite second spectral moment; retaining the full integral instead gives in that ideal continuum model.
Endpoint conditions also matter. If each end is moment-free and has no transverse applied force, the natural conditions from the variation areat each end. These can produce a free-end curvature boundary layer of width . For a constant intrinsic filament curvature , integration of the higher-order Euler-Lagrange equation with zero transverse force gives and henceThe last formula follows by integrating , and tends to , despite the vanishing bulk curvature gradient. Thus a finite free-ended measurement must include or suppress endpoint bending before interpreting a bulk fit.
For the freely jointed chain, rigid links have independent orientations, so the restoring force is entropic. Let now denote absolute temperature, and with Boltzmann constant . In the usual three-dimensional chain, a segment at polar angle has force energy . Its angular canonical partition function and the full chain partition function areDifferentiating with respect to yields the exact mean projected displacementHere is the Langevin function; this is force-extension of a three-dimensional freely jointed chain, in the fixed-force canonical ensemble. At high extension, , soThus the smooth quenched-curvature bulk deficit falls as , whereas the three-dimensional freely jointed chain deficit falls as and depends explicitly on temperature. The distinction is mechanical straightening of a fixed intrinsic shape versus orientational entropy; thermal bending fluctuations of a stiff filament have not been included in the first calculation.
If the comparison chain is also restricted to two dimensions, it is a planar freely jointed chain rather than the three-dimensional model. In this case,The last identity follows directly by differentiating the integral defining ; and are Modified Bessel functions of the first kind. At large the angular weight is proportional to , giving . Consequently : the same inverse-force exponent, with half the three-dimensional coefficient. Both versions assume inextensible links and forces below the regime where the links themselves stretch.