We describe a torsion pendulum with a large mass-quadrupole moment and a resonant frequency of 2.8 mHz, whose angle is measured using a Michelson interferometer. The system achieved noise levels of ∼200prad/Hz between 0.2 and 30 Hz and ∼10prad/Hz above 100 Hz. Such a system can be applied to a broad range of fields from the study of rotational seismic motion and elastogravity signals to gravitational wave observation and tests of gravity.
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http://dx.doi.org/10.1063/5.0043098 | DOI Listing |
Sensors (Basel)
December 2024
Space Environmental Load Engineering Center, Lanzhou Institute of Physics, Lanzhou 730000, China.
Sci Rep
November 2024
Khalifa University of Science and Technology, Abu Dhabi, United Arab Emirates.
The study presents a new configuration of nonlinear energy sinks (NESs) which is adaptable to function as either stable or bistable NES. The proposed NES is based on the spring-loaded inverted pendulum (SLIP) in which a torsional stiffness element couples the SLIP to the linear oscillator (LO). The bistable configuration provides a critically stable position when the SLIP is vertically aligned with respect to the LO motion.
View Article and Find Full Text PDFPhys Rev Lett
August 2024
Department of Physical Sciences, Indian Institute of Science Education and Research Mohali, Sector-81, Mohali 140306, India.
We show a new class of optical silk torsion pendulum (TOP) with zepto-Newton-meter (zNm) sensitivity achieved by exploiting hitherto unknown ultrasoft twist response of tough silk fibers in ultrahigh vacuum. We demonstrate several macroscopic microgram TOPs using three different silk types showing 6 orders of magnitude wide range of sensitivity calibrated using up to zNm optical torques. Remarkably, a nanoscale diameter capture silk exhibits about 20 fNm/rad torsion constant with low damping and responds to sub-400 zNm impulses over many oscillation cycles.
View Article and Find Full Text PDFSensors (Basel)
February 2024
Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China.
Inertial sensors are the key payloads in space gravitational wave detection missions, and they need to ensure that the test mass (TM), which serves as the inertial reference, freely floats in the spacecraft without contact, so that the TM is not disturbed by the satellite platform and the cosmic environment. Space gravitational wave detection missions require that the residual acceleration of the TM should be less than 3×10-15ms-2Hz-1/2. However, the TM with charges will interact with surrounding conductors and magnetic fields, introducing acceleration noise such as electrostatic force and Lorentz force.
View Article and Find Full Text PDFRev Sci Instrum
November 2023
MOE Key Laboratory of TianQin Mission, TianQin Research Center for Gravitational Physics & School of Physics and Astronomy, Frontiers Science Center for TianQin, Gravitational Wave Research Center of CNSA, Sun Yat-sen University (Zhuhai Campus), Zhuhai 519082, China.
Torsion pendulums are widely used for the measurement of small forces. In this study, we investigated the impact of temperature fluctuations on a torsion pendulum using heating devices to modulate the environmental temperature at different specific frequencies. The response coefficient between the temperature variation and the torque of the torsion pendulum was found to vary at different frequencies, with values from 4 × 10-15 N mK-1 at 0.
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