We investigate spontaneous emission from excitons beyond the point source dipole approximation and show how the symmetry of the exciton wave function plays a crucial role. We find that for spherically symmetric wave functions, the Purcell effect is independent of the wave function size and therefore is given exactly by the dipole approximation theory. This surprising result is a spontaneous emission counterpart to the shell theorems of classical mechanics and electrostatics and provides insights into the physics of mesoscopic emitters as well as great simplifications in practical calculations. DOI: 10.1103/PhysRevB.88.205308 PACS number(s): 42.50.−p, 42.70.Qs, 78.20.Bh, 78.67.Hc The Purcell effect is the relative change in the spontaneous emission decay rate of an excited emitter due to the photonic environment. While originally derived for optical microcavities, 1 the effect has been observed in a wide range of material systems including planar interfaces, 2 photonic crystals (PCs), 3 and near metal nanoparticles. 4 A recent application has been to employ a controlled Purcell effect for extracting fundamental properties of semiconductor quantum dots (QDs), such as the oscillator strength and the internal quantum efficiency. 5,6 By increasing the spontaneous emission rate, the Purcell effect can be utilized for overcoming the decoherence and dissipation processes inherent to QDs. For this reason, the Purcell effect has important applications in the generation of coherent photons from QDs 7 and in solid-state optical quantum processing in general, 8,9 and the Purcell effect remains a main driving force for nanophotonics research. Very large Purcell effects have been predicted for dipole emitters near nanoscale metal structures due to extreme field gradients, but recent studies have shown that nonlocal effects in the material response play a crucial role and that local theories can overestimate the Purcell effect by orders of magnitude.10 These results might suggest that nonlocal effects inside the emitter can smear out or average local variations in the photonic environment, e.g., near metallic nanostructures. Nevertheless, we prove a surprising theorem showing that for spherical emitters the nonlocal optical response inside the emitter cannot change the Purcell effect, and we illustrate that this result is remarkably robust against deviations from spherical symmetry. Interestingly, the theorem takes the form of a shell theorem for spontaneous emission.Theoretically, the description of spontaneous emission from QDs is often performed using a framework originally derived for atoms and ions. It relies on the celebrated dipole approximation (DA), which greatly simplifies the theoretical description of light-matter interaction in cases where the wavelength is large compared to the extent of the emitter. For such point sources, the spontaneous emission decay rate factorizes as DA (r 0 ) = α QD ρ(r 0 ), where α QD is intrinsic to the QD and ρ(r 0 ) is the local density of states (LDOS) 11,12 describing the photoni...