Optimization of high sensitivity parametric transducers for the Gravitational Wave detector "Mario Schenberg"
被引:0
作者:
Liccardo, V.
论文数: 0引用数: 0
h-index: 0
机构:
ITA, Sao Jose Dos Campos, SP, BrazilITA, Sao Jose Dos Campos, SP, Brazil
Liccardo, V.
[1
]
Ferreira, E. C.
论文数: 0引用数: 0
h-index: 0
机构:
INPE, Sao Jose Dos Campos, SP, BrazilITA, Sao Jose Dos Campos, SP, Brazil
Ferreira, E. C.
[2
]
Aguiar, O. D.
论文数: 0引用数: 0
h-index: 0
机构:
INPE, Sao Jose Dos Campos, SP, BrazilITA, Sao Jose Dos Campos, SP, Brazil
Aguiar, O. D.
[2
]
Oliveira, R. M.
论文数: 0引用数: 0
h-index: 0
机构:
INPE, Sao Jose Dos Campos, SP, BrazilITA, Sao Jose Dos Campos, SP, Brazil
Oliveira, R. M.
[2
]
机构:
[1] ITA, Sao Jose Dos Campos, SP, Brazil
[2] INPE, Sao Jose Dos Campos, SP, Brazil
来源:
ADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATION II
|
2016年
/
9912卷
关键词:
Antennas;
Instrument optimisation;
Cryogenic detectors;
Resonant Detectors;
Implantation;
Material treatment;
D O I:
10.1117/12.2235867
中图分类号:
TH7 [仪器、仪表];
学科分类号:
0804 ;
080401 ;
081102 ;
摘要:
Parametric transducers may be used to monitor vibrational modes of resonant-mass Gravitational Wave (GW) detectors. This work focuses on the development and optimization of electromechanical transducers for the brazilian GW detector "Mario Schenberg" We present the design and preliminary results for the optimization process of the last generation of the Schenberg parametric transduction system. Thanks to the results obtained from the last run of tests improvements for the transduction system will be planned and performed, in order to make the detector suitable for the searching of GW signals. The aim would be to obtain information about the direction and polarization of waves produced by astrophysical sources in the frequency bands of the spherical detector resonant modes.