Low-Frequency Noise Mitigation and Bandgap Engineering using Seismic Metamaterials for Terrestrial Gravitational Wave Observatories
arXiv:2301.04325 · doi:10.1093/ptep/ptad040
Abstract
Gravitational-wave now became one of the important observational methods for studying the Universe since its first detection. However, the ground-based observatories have an inherent barrier to their detection frequency band due to the seismic and gravity gradient noises nearby the perturbation of the surroundings. A recent intriguing development of artificial structures for media called metamaterial is opening a new branch of wave mechanics and its application in various fields, in particular, suggesting a novel way of mitigating noises by controlling the media structure for propagating waves. In this paper, we propose a novel framework for handling noises in ground-based gravitational wave detectors by using wave mechanics under metamaterial media. Specifically, we suggest an application of the bandgap engineering technique for mitigating the underground effects of acoustic noises resulting from the seismic vibration in the KAGRA gravitational wave observatory.
arXiv comment7pages, 5figures
References in corpus (10)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Characterization of the LIGO detectors during their sixth science run
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector
- Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
- Seismic gravity-gradient noise in interferometric gravitational-wave detectors
- Homogenization of quasiperiodic structures and two-scale cut-and-projection convergence
- Lunar Gravitational-Wave Antenna
- Space-borne Gravitational Wave Observatories
- Identifying multichannel coherent couplings and causal relationships in gravitational wave detectors