scholarly journals Pre-merger localization of eccentric compact binary coalescences with second-generation gravitational-wave detector networks

2014 ◽  
Vol 441 (3) ◽  
pp. 1934-1942 ◽  
Author(s):  
K. Kyutoku ◽  
N. Seto
Keyword(s):  
Gravitational Wave ◽  
Second Generation ◽  
Gravitational Wave Detector ◽  
Wave Detector ◽  
Compact Binary

Status of the Advanced Virgo gravitational wave detector

2017 ◽  
Vol 32 (28n29) ◽  
pp. 1744003 ◽  
Author(s):  
F. Acernese ◽  
T. Adams ◽  
K. Agatsuma ◽  
L. Aiello ◽  
A. Allocca ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Second Generation ◽  
Gravitational Wave Detector ◽  
Wave Detector

Advanced Virgo is the French–Italian second generation laser gravitational wave detector, successor of the Initial Virgo. This new interferometer keeps only the infrastructure of its predecessor and aims to be ten times more sensitive, with its first science run planned for 2017. This article gives an overview of the Advanced Virgo design and the technical choices behind it. Finally, the up-to-date progresses and the planned upgrade for the following years are detailed.

scholarly journals Advanced Virgo: a second-generation interferometric gravitational wave detector

2014 ◽  
Vol 32 (2) ◽  
pp. 024001 ◽  
Author(s):  
F Acernese ◽  
M Agathos ◽  
K Agatsuma ◽  
D Aisa ◽  
N Allemandou ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Second Generation ◽  
Gravitational Wave Detector ◽  
Wave Detector

scholarly journals China’s first step towards probing the expanding universe and the nature of gravity using a space borne gravitational wave antenna

2021 ◽  
Vol 4 (1) ◽  
Author(s):  
Keyword(s):  
Gravitational Wave ◽  
Hubble Constant ◽  
Gravitational Wave Detector ◽  
Expanding Universe ◽  
Satellite Mission ◽  
Gravitational Wave Detection ◽  
Wave Detection ◽  
Wave Detector ◽  
Wave Antenna ◽  
Gravitational Wave Antenna

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.

A noise model for the Brazilian gravitational wave detector  Mario Schenberg 

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