Pith. sign in

REVIEW 1 cited by

A Fermi-degenerate three-dimensional optical lattice clock

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1702.01210 v2 pith:6CXCJ3M6 submitted 2017-02-04 physics.atom-ph cond-mat.quant-gasquant-ph

classification physics.atom-phcond-mat.quant-gasquant-ph
keywords clocklatticeopticalshiftshighinteractionsthree-dimensionaltimes
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

Strontium optical lattice clocks have the potential to simultaneously interrogate millions of atoms with a high spectroscopic quality factor of $4 \times 10^{-17}$. Previously, atomic interactions have forced a compromise between clock stability, which benefits from a large atom number, and accuracy, which suffers from density-dependent frequency shifts. Here, we demonstrate a scalable solution which takes advantage of the high, correlated density of a degenerate Fermi gas in a three-dimensional optical lattice to guard against on-site interaction shifts. We show that contact interactions are resolved so that their contribution to clock shifts is orders of magnitude lower than in previous experiments. A synchronous clock comparison between two regions of the 3D lattice yields a $5 \times 10^{-19}$ measurement precision in 1 hour of averaging time.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites

    astro-ph.IM 2024-01 unverdicted novelty 7.0 of 10

    Proposes APTA with 6 satellites and 10^{-18} relative clock uncertainty at 1s averaging to achieve sensitivity for observing 10^3-10^4 solar-mass black hole mergers in the decihertz band.

Pith tools