Benefit of a larger detector array for prompt gravitational wave detection

Shin Kee Chung; Qi Chu; Shaun Hooper; Linqing Wen; Yuan Liu; Zhihui Du

doi:10.1142/9789814623995_0348

Benefit of a larger detector array for prompt gravitational wave detection

Shin Kee Chung, Qi Chu, Shaun Hooper, Linqing Wen, Yuan Liu, Zhihui Du

School of Physics, Mathematics and Computing

Research output: Chapter in Book/Conference paper › Conference paper › peer-review

Abstract

We are at the dawn of making the first detection of gravitational waves (GWs). The advanced LIGO and VIRGO detectors are funded and are under construction with a promise of a few of detections a year. A larger GW network is forming with the KA-GRA detector in Japan partially funded and LIGO-India on the near horizon. A low-latency search pipeline is crucial for enabling follow-up electromagnetic observation when a gravitational-wave signal is detected. In this paper, we discuss the benefit for a larger network that includes AIGO - a GW detector at the southern hemisphere for low-latency detections of gravitaional waves. The status of current low-latency search pipelines for GWs from compact binary coalescence will be presented.

Original language	English
Title of host publication	On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories
Editors	Kjell Rosquist, Robert T. Jantzen, Remo Ruffini, Remo Ruffini
Publisher	World Scientific Publishing
Pages	2029-2031
Number of pages	3
Edition	210699
ISBN (Print)	9789814612142
DOIs	https://doi.org/10.1142/9789814623995_0348
Publication status	Published - 1 Jan 2015
Event	13th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation, and Relativistic Field Theories, MG13 2012 - Stockholm, Sweden Duration: 1 Jul 2015 → 7 Jul 2015

Conference

Conference	13th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation, and Relativistic Field Theories, MG13 2012
Country/Territory	Sweden
City	Stockholm
Period	1/07/15 → 7/07/15

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10.1142/9789814623995_0348

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Chung, S. K., Chu, Q., Hooper, S., Wen, L., Liu, Y., & Du, Z. (2015). Benefit of a larger detector array for prompt gravitational wave detection. In K. Rosquist, R. T. Jantzen, R. Ruffini, & R. Ruffini (Eds.), On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories (210699 ed., pp. 2029-2031). World Scientific Publishing. https://doi.org/10.1142/9789814623995_0348

Chung, Shin Kee ; Chu, Qi ; Hooper, Shaun et al. / Benefit of a larger detector array for prompt gravitational wave detection. On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories. editor / Kjell Rosquist ; Robert T. Jantzen ; Remo Ruffini ; Remo Ruffini. 210699. ed. World Scientific Publishing, 2015. pp. 2029-2031

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title = "Benefit of a larger detector array for prompt gravitational wave detection",

abstract = "We are at the dawn of making the first detection of gravitational waves (GWs). The advanced LIGO and VIRGO detectors are funded and are under construction with a promise of a few of detections a year. A larger GW network is forming with the KA-GRA detector in Japan partially funded and LIGO-India on the near horizon. A low-latency search pipeline is crucial for enabling follow-up electromagnetic observation when a gravitational-wave signal is detected. In this paper, we discuss the benefit for a larger network that includes AIGO - a GW detector at the southern hemisphere for low-latency detections of gravitaional waves. The status of current low-latency search pipelines for GWs from compact binary coalescence will be presented.",

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author = "Chung, {Shin Kee} and Qi Chu and Shaun Hooper and Linqing Wen and Yuan Liu and Zhihui Du",

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doi = "10.1142/9789814623995_0348",

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publisher = "World Scientific Publishing",

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Chung, SK, Chu, Q, Hooper, S, Wen, L, Liu, Y & Du, Z 2015, Benefit of a larger detector array for prompt gravitational wave detection. in K Rosquist, RT Jantzen, R Ruffini & R Ruffini (eds), On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories. 210699 edn, World Scientific Publishing, pp. 2029-2031, 13th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation, and Relativistic Field Theories, MG13 2012, Stockholm, Sweden, 1/07/15. https://doi.org/10.1142/9789814623995_0348

Benefit of a larger detector array for prompt gravitational wave detection. / Chung, Shin Kee; Chu, Qi; Hooper, Shaun et al.
On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories. ed. / Kjell Rosquist; Robert T. Jantzen; Remo Ruffini; Remo Ruffini. 210699. ed. World Scientific Publishing, 2015. p. 2029-2031.

Research output: Chapter in Book/Conference paper › Conference paper › peer-review

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AU - Chung, Shin Kee

AU - Chu, Qi

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AB - We are at the dawn of making the first detection of gravitational waves (GWs). The advanced LIGO and VIRGO detectors are funded and are under construction with a promise of a few of detections a year. A larger GW network is forming with the KA-GRA detector in Japan partially funded and LIGO-India on the near horizon. A low-latency search pipeline is crucial for enabling follow-up electromagnetic observation when a gravitational-wave signal is detected. In this paper, we discuss the benefit for a larger network that includes AIGO - a GW detector at the southern hemisphere for low-latency detections of gravitaional waves. The status of current low-latency search pipelines for GWs from compact binary coalescence will be presented.

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BT - On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories

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Chung SK, Chu Q, Hooper S, Wen L, Liu Y, Du Z. Benefit of a larger detector array for prompt gravitational wave detection. In Rosquist K, Jantzen RT, Ruffini R, Ruffini R, editors, On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories. 210699 ed. World Scientific Publishing. 2015. p. 2029-2031 doi: 10.1142/9789814623995_0348

Benefit of a larger detector array for prompt gravitational wave detection

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