REVIEW 3 cited by
Tracing the redshift evolution of Hubble parameter with gravitational-wave standard sirens
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
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.
Forward citations
Cited by 3 Pith papers
-
Measuring the cosmic dipole with golden dark sirens in the era of next-generation ground-based gravitational wave detectors
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.
-
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range
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.
-
Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
The paper reviews cosmological tensions including the H0 and S8 discrepancies and explores new physics models that could explain them.
Discussion (0). Continue with ORCID to comment.