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Cosmography with the Einstein Telescope

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arxiv 0906.4151 v1 pith:53W4XUAG submitted 2009-06-23 astro-ph.CO gr-qc

B.S. Sathyaprakash (Cardiff University) , Bernard Schutz (MPI for Gravitational Physics - Albert Einstein Institute , Cardiff University) , Chris Van Den Broeck (Cardiff University) This is my paper · ORCID
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keywords darkeinsteinenergymergerstelescopeaccuratelybinarybursts
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Einstein Telescope (ET) is a 3rd generation gravitational-wave (GW) detector that is currently undergoing a design study. ET can detect millions of compact binary mergers up to redshifts 2-8. A small fraction of mergers might be observed in coincidence as gamma-ray bursts, helping to measure both the luminosity distance and red-shift to the source. By fitting these measured values to a cosmological model, it should be possible to accurately infer the dark energy equation-of-state, dark matter and dark energy density parameters. ET could, therefore, herald a new era in cosmology.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries

    gr-qc 2025-08 conditional novelty 6.0 of 10

    SEBOB combines an EOB inspiral with a BOB merger-ringdown to produce aligned-spin waveforms that match numerical relativity to about 2e-4 median mismatch, comparable to SEOBNRv5.

  2. Investigating the cosmic distance duality relation with gamma-ray bursts

    astro-ph.CO 2025-09 reject novelty 5.0 of 10

    Combined gamma-ray burst and multi-probe data show no significant violation of the cosmic distance duality relation and prefer a Planck-like Hubble constant.

  3. Science Case for the Einstein Telescope

    astro-ph.CO 2019-12 unverdicted novelty 3.0 of 10

    The Einstein Telescope will enable gravitational-wave observations up to cosmological distances, opening avenues for discoveries in astrophysics, cosmology, and fundamental physics.

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