Selective readout and back-action reduction for wideband acoustic gravitational wave detectors

被引:29
作者
Bonaldi, M [1 ]
Cerdonio, M
Conti, L
Pinard, M
Prodi, GA
Taffarello, L
Zendri, JP
机构
[1] CNR, ITC, Ist Foton & Nanotecnol, I-38050 Trent, Italy
[2] Ist Nazl Fis Nucl, I-38050 Trent, Italy
[3] Ist Nazl Fis Nucl, Padova Sect, I-35100 Padua, Italy
[4] Univ Padua, Dept Phys, I-35100 Padua, Italy
[5] Lab Kastler Brossel, F-75252 Paris, France
[6] Univ Trent, Dipartimento Fis, I-38050 Trent, Italy
来源
PHYSICAL REVIEW D | 2003年 / 68卷 / 10期
关键词
D O I
10.1103/PhysRevD.68.102004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the concept of the "selective readout" for the recently proposed dual detector [M. Cerdonio et al., Phys. Rev. Lett. 87, 031101 (2001)] of gravitational waves which is a sensitive and broadband resonant-mass detector. The advantage of the proposed detection scheme is that it is made sensitive only to the acoustic modes of the masses forming the detector that have quadrupolar symmetry, and thus carry the signal, while it rejects efficiently the noise contribution from the other modes, either of thermal or back-action origin. The total effect is that the sensitivity of a dual detector equipped with the selective readout is flat within a wide frequency range and can be as good as similar to8x10(-24)/rootHz between 1.3 and 4 kHz for a silicon carbide detector, 3 m in diameter.
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页数:6
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