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High-precision, Sagnac interferometry has long been proposed as a route to test fundamental questions in physics such as the magnitude of relativistic precessions (e.g., the Lense-Thirring effect). Although many elaborate experiments have been performed using, for example, matter wave interferometry or even quantum entanglement, none are within six orders of magnitude of the sensitivity and stability required to achieve such a measurement. We report on the operation of a free space ring laser gyroscope over a period of 250 days under an ambient pressure stabilizing vessel continuously in an unperturbed underground laboratory. Because we measure relative to local inertial space, the precession and nutation motion of Earth's axis are intrinsically contained in the observations. It is demonstrated that optical interferometry, using an ultrastable cavity, yields an accuracy limit for rotation sensing of 48 parts per billion (i.e., picoradians per second), less than an order of magnitude away from the regime in which relativistic effects can be measured.
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http://dx.doi.org/10.1126/sciadv.adx6634 | DOI Listing |
Sci Adv
September 2025
School of Physical and Chemical Sciences, University of Canterbury, Christchurch 8140, New Zealand.
High-precision, Sagnac interferometry has long been proposed as a route to test fundamental questions in physics such as the magnitude of relativistic precessions (e.g., the Lense-Thirring effect).
View Article and Find Full Text PDFAnal Chem
June 2025
Environmental NMR Centre, University of Toronto Scarborough, Toronto, ON M1C 1A4, Canada.
neonates and eggs are critical life stages that show different susceptibilities to toxins and stressors compared to adults. Nuclear magnetic resonance (NMR) spectroscopy has unique potential to uncover the underlying biochemical causes, but such very small, mass-limited samples are challenging to study. While the enhanced mass sensitivity of microcoils leads to markedly improved NMR analysis, experiments are often still long, leading to low throughput.
View Article and Find Full Text PDFJ Magn Reson
May 2024
Department of Chemistry, North Carolina State University, 2620 Yarbrough Dr., Raleigh, NC 27695, US. Electronic address:
One of the most essential prerequisites for the development of pulse Dynamic Nuclear Polarization (DNP) is the ability to generate high-power coherent mm-wave pulses at the electron precession frequencies corresponding to the magnetic fields of modern high-resolution NMR spectrometers. As a major step towards achieving this goal, an Extended Interaction Klystron (EIK) pulse amplifier custom-built by the Communications and Power Industries, Inc. and producing up to 140 W at 197.
View Article and Find Full Text PDFSensors (Basel)
December 2021
Department Section of Astronomy and Geodesy, Faculty of Mathematics, University Complutense of Madrid, E-28040 Madrid, Spain.
Very long baseline interferometry (VLBI) is the only technique in space geodesy that can determine directly the celestial pole offsets (CPO). In this paper, we make use of the CPO derived from global VLBI solutions to estimate empirical corrections to the main lunisolar nutation terms included in the IAU 2006/2000A precession-nutation model. In particular, we pay attention to two factors that affect the estimation of such corrections: the celestial reference frame used in the production of the global VLBI solutions and the stochastic model employed in the least-squares adjustment of the corrections.
View Article and Find Full Text PDFSci Adv
July 2021
Max Planck Institute for the Science of Light, Staudtstr. 2, 91058 Erlangen, Germany.
The complex tumbling motion of spinning nonspherical objects is a topic of enduring interest, both in popular culture and in advanced scientific research. Here, we report all-optical control of the spin, precession, and nutation of vaterite microparticles levitated by counterpropagating circularly polarized laser beams guided in chiral hollow-core fiber. The circularly polarized light causes the anisotropic particles to spin about the fiber axis, while, regulated by minimization of free energy, dipole forces tend to align the extraordinary optical axis of positive uniaxial particles into the plane of rotating electric field.
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