scholarly journals Data-analysis strategy for detecting gravitational-wave signals from inspiraling compact binaries with a network of laser-interferometric detectors

2001 ◽  
Vol 64 (4) ◽  
Author(s):  
Archana Pai ◽  
Sanjeev Dhurandhar ◽  
Sukanta Bose
Keyword(s):  
Data Analysis ◽  
Gravitational Wave ◽  
Compact Binaries ◽  
Analysis Strategy ◽  
Interferometric Detectors ◽  
Laser Interferometric

scholarly journals DETECTION OF GRAVITATIONAL WAVES FROM INSPIRALING, COMPACT BINARIES USING A NETWORK OF INTERFEROMETRIC DETECTORS

2000 ◽  
Vol 09 (03) ◽  
pp. 325-329 ◽  
Author(s):  
SUKANTA BOSE ◽  
ARCHANA PAI ◽  
SANJEEV DHURANDHAR
Keyword(s):  
Data Analysis ◽  
Gravitational Wave ◽  
Gravitational Waves ◽  
Analysis Problem ◽  
Compact Binaries ◽  
Correlation Vector ◽  
Compact Binary ◽  
Interferometric Detectors ◽  
First Time ◽  
Laser Interferometric

We formulate the data analysis problem for the detection of the Newtonian waveform from an inspiraling, compact binary by a network of arbitrarily oriented and arbitrarily located laser interferometric gravitational-wave detectors. We obtain for the first time the relation between the optimal statistic and the magnitude of the network correlation vector, which is constructed from the matched network-filter.

scholarly journals Coincidence and coherent data analysis methods for gravitational wave bursts in a network of interferometric detectors

2003 ◽  
Vol 68 (10) ◽  
Author(s):  
Nicolas Arnaud ◽  
Matteo Barsuglia ◽  
Marie-Anne Bizouard ◽  
Violette Brisson ◽  
Fabien Cavalier ◽  
...  
Keyword(s):  
Data Analysis ◽  
Gravitational Wave ◽  
Analysis Methods ◽  
Wave Bursts ◽  
Interferometric Detectors ◽  
Data Analysis Methods

scholarly journals MATCHING OF THE CONTINUOUS GRAVITATIONAL WAVE IN AN ALL SKY SEARCH

2003 ◽  
Vol 12 (07) ◽  
pp. 1227-1239 ◽  
Author(s):  
S. K. SAHAY
Keyword(s):  
Gravitational Wave ◽  
Source Location ◽  
The Other ◽  
Interferometric Detectors ◽  
Laser Interferometric

We investigate the matching of continuous gravitational wave (CGW) signals in an all sky search with reference to Earth based laser interferometric detectors. We consider the source location as the parameters of the signal manifold and templates corresponding to different source locations. It has been found that the matching of signals from locations in the sky that differ in their co-latitude and longitude by π radians decreases with source frequency. We have also made an analysis with the other parameters affecting the symmetries. We observe that it may not be relevant to take care of the symmetries in the sky locations for the search of CGW from the output of LIGO-I, GEO600 and TAMA detectors.

scholarly journals Gravitational-wave searches in the era of Advanced LIGO and Virgo

2021 ◽  
pp. 2130022
Author(s):  
Sarah Caudill ◽  
Shivaraj Kandhasamy ◽  
Claudia Lazzaro ◽  
Andrew Matas ◽  
Magdalena Sieniawska ◽  
...  
Keyword(s):  
Data Analysis ◽  
Gravitational Wave ◽  
Gravitational Waves ◽  
The United States ◽  
Compact Binary ◽  
Current State ◽  
Analysis Methods ◽  
Long Duration ◽  
Transient Sources ◽  
Interferometric Detectors

The field of gravitational-wave astronomy has been opened up by gravitational-wave observations made with interferometric detectors. This review surveys the current state-of-the-art in gravitational-wave detectors and data analysis methods currently used by the Laser Interferometer Gravitational-Wave Observatory in the United States and the Virgo Observatory in Italy. These analysis methods will also be used in the recently completed KAGRA Observatory in Japan. Data analysis algorithms are developed to target one of four classes of gravitational waves. Short duration, transient sources include compact binary coalescences, and burst sources originating from poorly modeled or unanticipated sources. Long duration sources include sources which emit continuous signals of consistent frequency, and many unresolved sources forming a stochastic background. A description of potential sources and the search for gravitational waves from each of these classes are detailed.

scholarly journals THE ROLE OF THE QUANTUM PROPERTIES OF GRAVITATIONAL RADIATION IN THE DETECTION OF GRAVITATIONAL WAVES

1999 ◽  
Vol 14 (13) ◽  
pp. 1997-2012 ◽  
Author(s):  
A. CAMACHO
Keyword(s):  
Gravitational Wave ◽  
Gravitational Radiation ◽  
Measuring Device ◽  
Quantum Properties ◽  
Large Dispersion ◽  
Experimental Apparatus ◽  
Definition Of ◽  
Interferometric Detectors ◽  
Laser Interferometric

The role that the quantum properties of a gravitational wave could play in the detection of gravitational radiation is analyzed. It is not only corroborated that in the current laser-interferometric detectors the resolution of the experimental apparatus could lie very far from the corresponding quantum threshold (thus the backreaction effect of the measuring device upon the gravitational wave is negligible), but it is also suggested that the consideration of the quantum properties of the wave could entail the definition of dispersion of the measurement outputs. This dispersion would be a function not only of the sensitivity of the measuring device, but also of the interaction time (between measuring device and gravitational radiation) and of the arm length of the corresponding laser interferometer. It would have a minimum limit, and the introduction of the current experimental parameters suggests that the dispersion of the existing proposals could lie very far from this minimum, which means that they would show a very large dispersion.

scholarly journals Laser-interferometric detectors for gravitational wave backgrounds at 100 MHz: Detector design and sensitivity

2008 ◽  
Vol 77 (2) ◽  
Author(s):  
Atsushi Nishizawa ◽  
Seiji Kawamura ◽  
Tomotada Akutsu ◽  
Koji Arai ◽  
Kazuhiro Yamamoto ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Interferometric Detectors ◽  
Laser Interferometric ◽  
Detector Design

scholarly journals Data analysis of massive gravitational waves from gamma ray bursts

2017 ◽  
Vol 26 (13) ◽  
pp. 1750150
Author(s):  
P. Prasia ◽  
V. C. Kuriakose
Keyword(s):  
Data Analysis ◽  
Bayesian Analysis ◽  
Gravitational Wave ◽  
Gravitational Waves ◽  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Massive Mode ◽  
Polarization Component ◽  
Current Configuration ◽  
Laser Interferometric

We investigate the detectability of massive mode of polarization of Gravitational Waves (GWs) in [Formula: see text] theory of gravity associated with Gamma Ray Bursts (GRBs) sources. We obtain the beam pattern function of Laser Interferometric Gravitational wave Observatory (LIGO) corresponding to the massive polarization of GWs and perform Bayesian analysis to study this polarization. It is found that the massive polarization component with a mass of [Formula: see text][Formula: see text]eV/c2 is too weak to be detected at LIGO with its current configuration.

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