Design and verification of low acoustic loss suspension systems for measuring the Q-factor of a gravitational wave detector test mass

1998 ◽  
Vol 246 (1-2) ◽  
pp. 37-42 ◽  
Author(s):  
Mitsuru Taniwaki ◽  
Li Ju ◽  
David G. Blair ◽  
Michael E. Tobar
2020 ◽  
Vol 102 (12) ◽  
Author(s):  
J. Eichholz ◽  
N. A. Holland ◽  
V. B. Adya ◽  
J. V. van Heijningen ◽  
R. L. Ward ◽  
...  

2021 ◽  
Vol 2090 (1) ◽  
pp. 012157
Author(s):  
A R C Prado ◽  
F S Bortoli ◽  
N. S. Magalhaes ◽  
R N Duarte ◽  
C Frajuca ◽  
...  

Abstract Interferometric gravitational wave detectors (IGWD) are a very complex detector, the need to lock the detector in a dark fringe condition besides the vibrations that affect the mirrors, creates the necessity of using active suspension systems. These active systems make the system reach the desired sensitivity but make the calibration of such detectors much more difficult. To solve this problem a calibrator is proposed, a resonant mass gravitational wave detector could be used to detect the same signal in a narrower band and use the measured amplitude to calibrate the IGWD, as resonant mass gravitational wave detectors are easily calibrated. This work aims to design the mechanical antenna of such a calibrator. The main difficulty is to design the calibrator is the frequencies required to make the detection. These massive detectors usually were made in frequencies close to 1 kHz and the frequency range to operate for better sensitivity is around 100 Hz. The antenna is modelled in finite elements method and a design of such an antenna is presented.


1995 ◽  
Vol 199 (5-6) ◽  
pp. 307-314 ◽  
Author(s):  
S. Braccini ◽  
C. Bradaschia ◽  
R. del Fabbro ◽  
A. di Virgilio ◽  
I. Ferrante ◽  
...  

2021 ◽  
Vol 4 (1) ◽  
Author(s):  

AbstractIn this perspective, we outline that a space borne gravitational wave detector network combining LISA and Taiji can be used to measure the Hubble constant with an uncertainty less than 0.5% in ten years, compared with the network of the ground based gravitational wave detectors which can measure the Hubble constant within a 2% uncertainty in the next five years by the standard siren method. Taiji is a Chinese space borne gravitational wave detection mission planned for launch in the early 2030 s. The pilot satellite mission Taiji-1 has been launched in August 2019 to verify the feasibility of Taiji. The results of a few technologies tested on Taiji-1 are presented in this paper.


2004 ◽  
Vol 21 (5) ◽  
pp. S1107-S1111 ◽  
Author(s):  
Carlos Frajuca ◽  
Kilder L Ribeiro ◽  
Luiz A Andrade ◽  
Odylio D Aguiar ◽  
Nadja S Magalhães ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document