This articlerelies largely or entirely on asingle source. Relevant discussion may be found on thetalk page. Please helpimprove this article byintroducing citations to additional sources. Find sources: "Torsion-bar antenna" – news ·newspapers ·books ·scholar ·JSTOR(February 2016) |
Atorsion-bar antenna (TOBA) is a novel scheme for agravitational wave detector, proposed by M. Ando, et al. in 2010. The proposed design is composed of two, long, thin bars, suspended as torsion pendula in a cross-like fashion. Their differential angle (sensitive to tidalgravitational wave forces) would be compared using a set of optical cavities with one end mirror of each cavity fixed to the ends of each bar. Such a detector could be fashioned either for ground-based or space-based use.
The predicted frequency band over which such a detector would be most sensitive would be centered on 1 Hz, similar toDECIGO. This frequency range would complement current ground-based, laser interferometric detectors (whose sensitive band is between 10–100 Hz and several kHz, such asLIGO orVirgo), and proposed space-based, laser interferometric detectors (such asLISA whose sensitive band is centered on 10−4 Hz).[1]
Thisrelativity-related article is astub. You can help Wikipedia byexpanding it. |