Exploring the Sensitivity of Next Generation Gravitational Wave Detectors - INSPIRE

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Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

LIGO Scientific

Collaboration

Jul 29, 2016

18 pages

Published in:

Class.Quant.Grav. 34 (2017) 4, 044001

Published: Jan 24, 2017

e-Print:

1607.08697 [astro-ph.IM]

DOI:

10.1088/1361-6382/aa51f4

Report number:

LIGO-P1600143

Experiments:

LIGO

View in:

reference search1,218 citations

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Abstract: (arXiv)

The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.

Note:

Withdrawn due to author list discussion

binary: compact
target: design
gravitational radiation detector
gravitational radiation
detector: sensitivity
LIGO

References(75)

Figures(0)

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