A perturbation-theory treatment of gravitational waves in a Robertson-Walker universe yields a next-to-leading-order correction factor to the waveform, but the quantitative expression appears to contain sign and factor errors.
Somiya and (for the KAGRA Collabo- ration), Detector configuration of kagra–the japanese cryogenic gravitational-wave detector, Classical and Quantum Gravity 29, 124007 (2012)
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
citation-role summary
background 1
citation-polarity summary
fields
gr-qc 1years
2024 1verdicts
REJECT 1roles
background 1polarities
background 1representative citing papers
citing papers explorer
-
The imprint of cosmic expansion history on the propagation of gravitational waves
A perturbation-theory treatment of gravitational waves in a Robertson-Walker universe yields a next-to-leading-order correction factor to the waveform, but the quantitative expression appears to contain sign and factor errors.