Accurate precision cosmology with redshift unknown gravitational wave sources

@article{Mukherjee2021AccuratePC,
  title={Accurate precision cosmology with redshift unknown gravitational wave sources},
  author={Suvodip Mukherjee and Benjamin D. Wandelt and Samaya M. Nissanke and Alessandra Silvestri},
  journal={Physical Review D},
  year={2021},
  volume={103},
  pages={043520}
}
Gravitational waves can provide an accurate measurement of the luminosity distance to the source but cannot provide the source redshift unless the degeneracy between mass and redshift can be broken. This makes it essential to infer the redshift of the source independently to measure the expansion history of the Universe. We show that by exploiting the clustering scale of the gravitational wave sources with galaxies of a known redshift, we can infer the expansion history from redshift unknown… 

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References

SHOWING 1-10 OF 190 REFERENCES
"J."
however (for it was the literal soul of the life of the Redeemer, John xv. io), is the peculiar token of fellowship with the Redeemer. That love to God (what is meant here is not God’s love to men)
Astrophys
  • J. 876, 85
  • 2019
MNRAS 227
  • 1
  • 1987
d.
The Large-Scale Structure of the Universe
Opinions on the large-scale structure of the early universe range widely from primeval chaos to a well-ordered mass distribution. P.J.E. Peebles argues that the evolution proceeded from a nearly
Characterization of systematic error in Advanced LIGO calibration
The raw outputs of the detectors within the Advanced Laser Interferometer Gravitational-Wave Observatory need to be calibrated in order to produce the estimate of the dimensionless strain used for
DES, LIGO Scientific, Virgo), Astrophys
  • J. Lett. 876,
  • 2019
The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
We present a new and independent determination of the local value of the Hubble constant based on a calibration of the Tip of the Red Giant Branch (TRGB) applied to Type Ia supernovae (SNeIa). We
Nature 562
  • 545
  • 2018
Phys
  • Rev. D 98, 023502
  • 2018
...
1
2
3
4
5
...