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Tracing the redshift evolution of Hubble parameter with gravitational-wave standard sirens

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arxiv 1011.5000 v2 pith:LP5S32BH submitted 2010-11-23 astro-ph.CO

classification astro-ph.CO
keywords redshiftdistancehubbleluminosityparameterbinariesgravitational-wavehigh
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Proposed space-based gravitational-wave detectors such as BBO and DECIGO can detect ~10^6 neutron-star binaries and determine luminosity distance to the binaries with a high precision. Combining the luminosity distance and electromagnetically-derived redshift, one would be able to probe cosmological expansion out to high redshift. In this paper, we show that the Hubble parameter as a function of redshift can be directly measured with monopole and dipole components of the luminosity distance on the sky. As a result, the measurement accuracies of the Hubble parameter in each redshift bin up to z=1 are 3-14 %, 1.5-8 %, and 0.8-4% for the observation time 1 yr, 3 yr, and 10 yr, respectively.

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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. Measuring the cosmic dipole with golden dark sirens in the era of next-generation ground-based gravitational wave detectors

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Golden dark sirens from next-generation gravitational-wave networks could constrain the cosmic dipole amplitude to about 10^-3 jointly with H0 and to about 10^-4 if H0 is fixed.

  2. The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range

    gr-qc 2019-08 accept novelty 3.0 of 10

    A Decihertz Observatory would fill the gap between LISA and ground detectors, enabling early-warning multimessenger astronomy and measurements of intermediate-mass black hole populations.

  3. Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

    astro-ph.CO 2022-03 accept novelty 2.0 of 10

    The paper reviews cosmological tensions including the H0 and S8 discrepancies and explores new physics models that could explain them.

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