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Cosmography with the Einstein Telescope

Open access
Sathyaprakash, B S, Schutz, B F, Van Den Broeck, C·2010·Classical and Quantum Gravity

Abstract

The Einstein Telescope, a third-generation gravitational-wave detector under a design study, could detect millions of binary neutron star inspirals each year. A small fraction of these events might be observed as gamma-ray bursts, helping to measure both the luminosity distance D L to and redshift of the source. By fitting these measured values of D L and to a cosmological model, it would be possible to infer the dark energy equation of state to within 1.5% without the need to correct for errors in D L caused by weak lensing. This compares favourably with 0.3–10% accuracy that can be achieved with the Laser Interferometer Space Antenna (where weak lensing will need to be dealt with) as well as with dedicated dark energy missions that have been proposed, where 3.5–11% uncertainty is expected.

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Metadata

Authors
Sathyaprakash, B. S., Schutz, B. F., & Van Den Broeck, C.
Venue
Classical and Quantum Gravity
Published
2010-09-27
Volume
27
Issue
21
Pages
215006
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2169676629
Cited by
233
References
1
FWCI
4.92
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Cosmography with the Einstein Telescope. https://app.cochat.ai/papers/10.1088/0264-9381/27/21/215006
The paper
Sathyaprakash, B. S., Schutz, B. F., & Van Den Broeck, C. (2010). Cosmography with the Einstein Telescope. Classical and Quantum Gravity. https://doi.org/10.1088/0264-9381/27/21/215006

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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