Elastic rods and elastic spinning rings as gravitational wave detectors

Abstract Linearised relativistic elasticity equations of motion are considered for a rod and a spinning ring encountering a gravitational wave. In the case of the rod, the equations reduce to a wave equation with appropriate boundary conditions. Using Fourier transforms, the resonant frequencies are found and an explicit distributional solution is given, both for a plus- and a cross-polarised gravitational wave. In the case of the spinning ring, the equations are coupled wave equations with periodic boundary conditions. Using a Fourier series expansion, the system of wave equations is recast as a family of ordinary differential equations for the Fourier coefficients, which are then solved via Fourier transforms. The resonant frequencies are found, including simple approximate expressions for slowly rotating rings, and an explicit distributional solution is obtained in the case of the non-spinning ring. Interestingly, it is possible to tune the resonant frequencies by adjusting the angular velocity of the spinning ring.

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Publication Details

Journal
Zeitschrift für angewandte Mathematik und Physik
Published
2025-03-27
DOI
https://doi.org/10.1007/s00033-025-02461-6
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00

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article

Elastic rods and elastic spinning rings as gravitational wave detectors

Rodrigo Vicente, José Natário, Amol Sasane
Zeitschrift für angewandte Mathematik und Physik
Pulsars and Gravitational Waves Research
article

Elastic rods and elastic spinning rings as gravitational wave detectors

Rodrigo Vicente, José Natário, Amol Sasane
article en

Abstract

Abstract Linearised relativistic elasticity equations of motion are considered for a rod and a spinning ring encountering a gravitational wave. In the case of the rod, the equations reduce to a wave equation with appropriate boundary conditions. Using Fourier transforms, the resonant frequencies are found and an explicit distributional solution is given, both for a plus- and a cross-polarised gravitational wave. In the case of the spinning ring, the equations are coupled wave equations with periodic boundary conditions. Using a Fourier series expansion, the system of wave equations is recast as a family of ordinary differential equations for the Fourier coefficients, which are then solved via Fourier transforms. The resonant frequencies are found, including simple approximate expressions for slowly rotating rings, and an explicit distributional solution is obtained in the case of the non-spinning ring. Interestingly, it is possible to tune the resonant frequencies by adjusting the angular velocity of the spinning ring.

Zeitschrift für angewandte Mathematik und PhysikVol. 76(2)
University of Lisbon (PT), Institute for High Energy Physics (ES), London School of Economics and Political Science (GB)
Fundação para a Ciência e a Tecnologia
Openalex Percentile: Top 95%
Pulsars and Gravitational Waves Research
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