Abstract

High-resolution imaging of ultracold atoms typically requires custom high numerical aperture (NA) optics, as is the case for quantum gas microscopy. These high NA objectives involve many optical elements, each of which contributes to loss and light scattering, making them unsuitable for quantum backaction limited "weak" measurements. We employ a low-cost high NA aspheric lens as an objective for a practical and economical-although aberrated-high-resolution microscope to image 87Rb Bose-Einstein condensates. Here, we present a methodology for digitally eliminating the resulting aberrations that is applicable to a wide range of imaging strategies and requires no additional hardware. We recover nearly the full NA of our objective, thereby demonstrating a simple and powerful digital aberration correction method for achieving optimal microscopy of quantum objects. This reconstruction relies on a high-quality measure of our imaging system's even-order aberrations from density-density correlations measured with differing degrees of defocus. We demonstrate our aberration compensation technique using phase-contrast imaging, a dispersive imaging technique directly applicable to quantum backaction limited measurements. Furthermore, we show that our digital correction technique reduces the contribution of photon shot noise to density-density correlation measurements which would otherwise contaminate the desired quantum projection noise signal in weak measurements.

Highlights

  • In many fields of study—from biophysics [1] and medicine to astrophysics [2,3] and atomic physics [4]—images are a key source of data, making high-quality imaging systems essential

  • Our power spectral density (PSD) measurements exhibit additional structures, and we focus on the pair at positive ky giving additional limits to the effective vertical numerical aperture (NA)

  • We presented a versatile high-resolution ultracold atom microscope composed of two main components: (i) an economical and practical imaging system based on high NA off-the-shelf optics, and (ii) a high-fidelity digital aberration removal technique that is compatible with a wide range of imaging techniques

Read more

Summary

FUNDAMENTALS OF LIGHT-WAVE–MATTER INTERACTIONS

The majority of ultracold atom measurements rely on images of light that has interacted with an atomic ensemble. We summarize the theoretical description of laser light propagating along ez through a dilute atomic cloud: a nonpermeable dielectric medium. We relate the absorption and phase shift of the incident laser to a fundamental quantity in ultracold atom experiments: the 2D column density ρ2D(r⊥) = ρ(r)dz, where ρ(r) is the 3D atomic density with spatial coordinates r = xex + yey + zez and transverse coordinates r⊥ = xex + yey

The paraxial Helmholtz equation
Depth-of-field effects
Atomic susceptibility
IMAGING TECHNIQUES WITH COLD ATOMS
Phase-contrast imaging
Principle of phase-contrast imaging
Phase-contrast imaging with ultracold atoms
Absorption imaging
Aberrations
Signal-to-noise ratio
REGULARIZATION
Bayesian framework
Specific implementation
Spectral Tikhonov from uniform uncertainties
Ad hoc convolution approximation
Full method
Numerical comparison
ULTRACOLD ATOM MICROSCOPE
EXPERIMENTAL RESULTS
Fourier pupil function measurements
Correlations fit function
Density correlation measurements
Determining antisymmetric pupil phase contributions
Final pupil model
Digitally enhanced nondestructive imaging with far-detuned PCI
CONCLUSION AND OUTLOOK

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.