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Superresolution imaging with entanglement-enhanced telescopy

Isack Padilla, Aqil Sajjad, Babak N. Saif, Saikat Guha

Abstract

Long-baseline interferometry will be possible using pre-shared entanglement between two telescope sites to mimic the standard phase-scanning interferometer, but without physical beam combination. We show that spatial-mode sorting at each telescope, along with pre-shared entanglement, can be used to realize the most general multimode interferometry on light collected by any number of telescopes, enabling achieving quantitative-imaging performance at the ultimate limit pursuant to the baseline as afforded by quantum theory. We work out an explicit example involving two telescopes imaging two point sources.

Superresolution imaging with entanglement-enhanced telescopy

Abstract

Long-baseline interferometry will be possible using pre-shared entanglement between two telescope sites to mimic the standard phase-scanning interferometer, but without physical beam combination. We show that spatial-mode sorting at each telescope, along with pre-shared entanglement, can be used to realize the most general multimode interferometry on light collected by any number of telescopes, enabling achieving quantitative-imaging performance at the ultimate limit pursuant to the baseline as afforded by quantum theory. We work out an explicit example involving two telescopes imaging two point sources.

Paper Structure

This paper contains 17 equations, 2 figures.

Figures (2)

  • Figure 1: (a) A two-telescope array of baseline $b$ points toward two weakly emitting stars of angular separation $2\theta$. A star photon arriving at site A is shown. (b) The incoming photon is fed into a spatial mode demultiplexer (SPADE). An excitation is shown to occur in the second mode basis and in the fifth time bin of a block of integration time in which roughly one photon arrives. (c) The photonic state is loaded into the memory qubits via photon-memory CNOT gates, a compressive binary encoding, and performing X-basis measurements on the photon. (d) Entangled pairs pre-distributed among the telescope sites assist in performing a sequence of operations that reveal the arrival time and spatial mode index, which combined with (e) The X measurement results of relevant memory atoms, resuls in a single-bit post-processed outcome whose empirical probability over measurements of many time blocks containing one photon each, is the sufficient statistic to estimate $\theta$ at the QFI-mandated precision limit.
  • Figure 2: CFI normalized to the QFI, plotted as a color chart, versus separation $\theta/\sigma$ and baseline to aperture-diameter ratio $r$. Four values of the spatial-mode cuffoff $K$ are shown, with the top right corresponding to a binary SPADE ($K=2$) attaining the QFI in the sub-Rayleigh regime ($\theta/\sigma < 1$).