Non-fundamental noise sources

Stefan Ballmer, Bas Swinkels

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

Whereas the challenge to detect the elusive gravitational-wave signal drives the technological design of laser-interferometer gravitational-wave detectors, the identification and characterization of astrophysical sources emitting the gravitational-wave signals require a global network of gravitational-wave detectors. Using the simultaneous observations of a network of detectors has strong scientific motivations: (i) to increase the detection confidence of weak and rare gravitational-wave signals expected to be associated with highly energetic astrophysical phenomena, (ii) to improve signal/source reconstruction and then provide an accurate estimate of the source parameters, and (iii) to enable gravitational waves to be part of the multi-messenger observations of the Universe. It was, indeed, the network of the LIGO interferometers that detected and characterized the first gravitational-wave signals coming from binary black-hole mergers [Abbott et al. (2016c, e, 2017c, d)], opening a new channel for the exploration of the Universe. It was also the network of the LIGO and Virgo interferometers that detected and characterized the first gravitational-wave signal coming from a binary neutron star coalescence [Abbott et al. (2017f)], starting the era of multi-messenger astronomy including gravitational waves [Abbott et al. (2017g)]. This chapter focuses on the importance of a network of gravitational-wave detectors for gravitational-wave detection, gravitational-wave astrophysics and multi-messenger astronomy.

Original languageEnglish (US)
Title of host publicationAdvanced Interferometric Gravitational-Wave Detectors
Subtitle of host publicationIn 2 Volumes
PublisherWorld Scientific Publishing Co.
Pages185-196
Number of pages12
Volume1
ISBN (Electronic)9789813146082
ISBN (Print)9789813146075
DOIs
StatePublished - Jan 1 2019

Fingerprint

gravitational waves
astrophysics
LIGO (observatory)
interferometers
detectors
astronomy
universe
binary stars
coalescing
neutron stars
confidence

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Ballmer, S., & Swinkels, B. (2019). Non-fundamental noise sources. In Advanced Interferometric Gravitational-Wave Detectors: In 2 Volumes (Vol. 1, pp. 185-196). World Scientific Publishing Co.. https://doi.org/10.1142/9789813146082_0007

Non-fundamental noise sources. / Ballmer, Stefan; Swinkels, Bas.

Advanced Interferometric Gravitational-Wave Detectors: In 2 Volumes. Vol. 1 World Scientific Publishing Co., 2019. p. 185-196.

Research output: Chapter in Book/Report/Conference proceedingChapter

Ballmer, S & Swinkels, B 2019, Non-fundamental noise sources. in Advanced Interferometric Gravitational-Wave Detectors: In 2 Volumes. vol. 1, World Scientific Publishing Co., pp. 185-196. https://doi.org/10.1142/9789813146082_0007
Ballmer S, Swinkels B. Non-fundamental noise sources. In Advanced Interferometric Gravitational-Wave Detectors: In 2 Volumes. Vol. 1. World Scientific Publishing Co. 2019. p. 185-196 https://doi.org/10.1142/9789813146082_0007
Ballmer, Stefan ; Swinkels, Bas. / Non-fundamental noise sources. Advanced Interferometric Gravitational-Wave Detectors: In 2 Volumes. Vol. 1 World Scientific Publishing Co., 2019. pp. 185-196
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