📝 SummarXiv

Abstract

The Rayleigh diffraction limit imposes a fundamental restriction on the resolution of direct imaging systems, hindering the identification of incoherent optical sources, such as celestial bodies in astronomy and fluorophores in bioimaging. Recent advances in quantum sensing have shown that this limit can be circumvented through spatial demultiplexing (SPADE) and photon detection. Notably, the latter is a semi-classical detection strategy, being SPADE a linear transformation of the field and photon detection a measurement of intensity. However, the general optimality for arbitrary intensity distributions and bright sources remains unproven. In this work, we develop a general model for incoherent light with arbitrary intensity collected by passive, linear optical systems. We employ this framework to compute the quantum Chernoff exponent for generic incoherent-source discrimination problems, and we analyze several special cases, with particular focus on the subdiffraction regime for Gaussian point-spread functions. We show that, surprisingly, SPADE measurements do not always saturate the quantum Chernoff bound in the subdiffraction regime; the quantum optimality holds only when certain compatibility conditions, such as covariance matrix commutativity, are met. These findings suggest that collective measurements may actually be needed to achieve the ultimate quantum Chernoff bound for the discrimination of specific incoherent sources. For the fully general case, our analysis can still be used to find the best SPADE configurations, generally achieved through a hypotheses-dependent rotation of the SPADE modes. Our results advance the theory of quantum-limited optical discrimination, with possible applications in diagnostics, automated image interpretation, and galaxy identification.