2021
DOI: 10.1093/mnras/stab165
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Cosmology with the Einstein telescope: No Slip Gravity model and redshift specifications

Abstract: The Einstein Telescope and other third generation interferometric detectors of gravitational waves are projected to be operational post 2030. The cosmological signatures of gravitational waves would undoubtedly shed light on any departure from the current gravitational framework. We here confront a specific modified gravity model, the No Slip Gravity model, with forecast observations of gravitational waves. We compare the predicted constraints on the dark energy equation of state parameters $w_0^{}-w_a^{}$, be… Show more

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Cited by 21 publications
(17 citation statements)
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“…We find that the free parameter that quantifies deviation of GR, ξ, can be measured with 33%, 21% and 41% accuracy from the Pop III, Delay and No Delay populations, respectively. As already pointed out in [71], we see a significant degeneracy between the parameters ξ and n, which on the other hand is also very degenerate with the matter density Ω m and the Hubble constant, H 0 . Note that for n = 0, the equations of the model also reduces to GR.…”
Section: Resultssupporting
confidence: 73%
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“…We find that the free parameter that quantifies deviation of GR, ξ, can be measured with 33%, 21% and 41% accuracy from the Pop III, Delay and No Delay populations, respectively. As already pointed out in [71], we see a significant degeneracy between the parameters ξ and n, which on the other hand is also very degenerate with the matter density Ω m and the Hubble constant, H 0 . Note that for n = 0, the equations of the model also reduces to GR.…”
Section: Resultssupporting
confidence: 73%
“…Therefore, in this case, it will be important to combine the SS sample We have extended the analysis in Ref. [71] considering mock data from the LISA perspective. We see an overall improvement on the precision of the Hubble constant, H 0 , and Ω m by including the CMB information.…”
Section: Resultsmentioning
confidence: 99%
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“…In the future, it will be interesting to apply further constraints from upcoming future survey data [72,73] and other probes, such as clustering, FRB [74], and gravitational waves [75] and to examine the allowed range for the anomalous dimension η, which is related to the free parameter b = 2 − η in the model [7].…”
Section: Discussionmentioning
confidence: 99%