Initial operation of theM=390 kg cryogenic gravitational-wave antenna

1978 ◽  
Vol 1 (6) ◽  
pp. 497-509 ◽  
Author(s):  
E. Amaldi ◽  
C. Cosmelli ◽  
S. Frasca ◽  
I. Modena ◽  
G. V. Pallottino ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Initial Operation ◽  
Wave Antenna ◽  
Gravitational Wave Antenna

Initial operation at liquid-helium temperature of theM=2270 kg Al 5056 gravitational-wave antenna of the Rome group

1984 ◽  
Vol 7 (3) ◽  
pp. 338-354 ◽  
Author(s):  
E. Amaldi ◽  
E. Coccia ◽  
C. Cosmelli ◽  
Y. Ogawa ◽  
G. Pizzella ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Liquid Helium ◽  
Liquid Helium Temperature ◽  
Helium Temperature ◽  
Initial Operation ◽  
Wave Antenna ◽  
Gravitational Wave Antenna

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.

Virgo: Very wide band interferometric gravitational wave antenna

1992 ◽  
Vol 28 (1) ◽  
pp. 54-60 ◽  
Author(s):  
C. Bradaschia ◽  
R. Del Fabbro ◽  
A. Di Virgilio ◽  
R. Flaminio ◽  
S. Galeotti ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Wide Band ◽  
Wave Antenna ◽  
Gravitational Wave Antenna

HiSPARC AND MiniGRAIL

2005 ◽  
Vol 20 (29) ◽  
pp. 6884-6886 ◽  
Author(s):  
G. FROSSATI ◽  
C. T. HERBSCHLEB ◽  
J. B. R. OONK ◽  
A. DE WAARD
Keyword(s):  
High School ◽  
The Netherlands ◽  
Gravitational Wave ◽  
Cosmic Ray ◽  
High Energy ◽  
Large Array ◽  
School Project ◽  
Wave Antenna ◽  
Scientific Institutions ◽  
Gravitational Wave Antenna

HiSPARC (High-School Project on Astrophysics Research with cosmics) is a project that envisages the use of a large array of cosmic ray detectors placed at high-schools and scientific institutions in the Netherlands in order to measure high-energy cosmic ray showers. Besides contributing to the HiSPARC project, Leiden University also uses the cosmic ray detectors as veto for the resonant gravitational wave antenna MiniGRAIL.

scholarly journals Fake signals caused by heavy-mass motions near a sensitive spherical gravitational wave antenna

2002 ◽  
Vol 19 (19) ◽  
pp. 4845-4854
Author(s):  
Alberto Lobo ◽  
Massimo Cerdonio ◽  
 lvaro Montero
Keyword(s):  
Gravitational Wave ◽  
Wave Antenna ◽  
Gravitational Wave Antenna

DECIGO: THE JAPANESE SPACE GRAVITATIONAL WAVE ANTENNA

2008 ◽  
Author(s):  
MASAKI ANDO ◽  
SEIJI KAWAMURA ◽  
TAKASHI NAKAMURA ◽  
NAOKI SETO ◽  
KIMIO TSUBONO ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Wave Antenna ◽  
Gravitational Wave Antenna

Detection of massive Gravitational Waves using spherical antenna

2014 ◽  
Vol 23 (05) ◽  
pp. 1450037 ◽  
Author(s):  
P. Prasia ◽  
V. C. Kuriakose
Keyword(s):  
Gravitational Wave ◽  
Gravitational Waves ◽  
Mechanical Resonators ◽  
Spherical Antenna ◽  
Wave Antenna ◽  
Gravitational Wave Antenna ◽  
Theory Of Gravity

The generation of massive Gravitational Waves (GW) from metric f(R) theory of gravity is studied and the sensitivity of a spherical antenna detector towards such a wave is looked into. The energy sensitivity is maximum for the monopole mode of the sphere. Of the five quadrupole modes of a sphere, only three are triggered by a massive wave. Also, the sensitivity of a spherical antenna with mechanical resonators attached to it is studied. The Truncated Icosahedral Gravitational wave Antenna (TIGA), originally proposed for detecting the effect of massless GW on the quadrupole modes of a sphere, has been modified in this paper to get a Modified TIGA, in order to detect the sensitivity of monopole modes towards a massive wave.

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