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Words near each other
・ Torsion box
・ Torsion coefficient (topology)
・ Torsion conjecture
・ Torsion constant
・ Torsion dystonia
・ Torsion field
・ Torsion field (pseudoscience)
・ Torsion group
・ Torsion of a curve
・ Torsion pendulum clock
・ Torsion sheaf
・ Torsion siege engine
・ Torsion spring
・ Torsion subgroup
・ Torsion tensor
Torsion-Bar Antenna
・ Torsion-free
・ Torsion-free abelian group
・ Torsion-free abelian groups of rank 1
・ Torsion-free module
・ Torsional strain
・ Torsional vibration
・ Torsionless module
・ Torsk
・ Torsken
・ Torsken (village)
・ Torsken Church
・ Torslanda
・ Torslanda Airport
・ Torslanda Church


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Torsion-Bar Antenna : ウィキペディア英語版
Torsion-Bar Antenna
A torsion-bar antenna (or TOBA) is a novel scheme for a gravitational 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 tidal gravitational wave forces) would be compared using a set of optical cavities with one end mirror of each cavity fixed two the ends of the 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 band would be centered on 1 Hz, similar to DECIGO. This frequency range would complement current ground-based, laser interferometric detectors (whose sensitive band is between 10–100 Hz and several kHz, such as LIGO or Virgo), and proposed space-based, laser interferometric detectors (such as LISA whose sensitive band is centered on 10−4 Hz).
== References ==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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