Past exam of the mathematics course of the University of Cambridge 2009 ii Paper 1 38A Solution Created 2026-09-24 Updated 2026-10-14
For spherical symmetry, satisfies the one-dimensional wave equation, so an outgoing solution has the form . To relate to the source, use a velocity potential with and . The outgoing monopole potentialhas as , fixing its mass-flux normalization. It follows thatFor an element with displacement , its volume outflow is and mass outflow is times this. Thus . A rigid wall imposes zero normal velocity away from the source. The method of images uses a source of the same sign on the other side; a source on the plane and its image coincide, doubling the full-space monopole field. Equivalently its mass flux spreads over a hemisphere rather than a sphere. HenceThe small patch relative to wavelength justifies the point source, and the small displacement justifies linear acoustics.
Superposition over the aperture gives the Rayleigh integral for baffled acoustic radiationFor , and . The additional condition makes the omitted phase small, so with the printed Fourier transform conventionThe minus signs in arise because the outgoing phase contributes .
For the rectangle the two integrals factor, givingwhere and its zero-argument limit is one. If , implies , so the -direction factor is nearly one throughout the radiation hemisphere. With of order one the -direction factor varies appreciably: the long dimension gives stronger directivity in that angular direction, while the short dimension radiates broadly. The forward amplitude is proportional to the area . Nulls have equal to nonzero integer multiples of when those values are physically accessible; order-one does not automatically imply that the first null lies in the hemisphere.