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- W3042763725 abstract "We investigate how the propagation of an astrophysical gravitational wave background (AGWB) is modified over cosmological volumes when considering theories beyond general relativity of the type Horndeski gravity. We first deduce an amplitude correction on the AGWB induced for the presence of a possible running in the Planck mass. Then, we apply the spectral noise density from some ground-based interferometers, namely, the Advanced LIGO (aLIGO), Einstein Telescope (ET) and Cosmic Explore (CE), to evaluate the signal-to-noise ratio (SNR) as a function of the amplitude of the running of the Planck mass for two different scenarios. We find that for observation time period $gtrsim$ 5 yrs and $gtrsim$ 1 yr, we can have a significant signal of the AGWB in the band [1-100] Hz from the ET and CE sensitivity, respectively. Using Fisher information, we find some forecast bounds, and we deduce $lesssim$ 27% and $lesssim$ 18% correction at 1$sigma$ confidence level on the amplitude of the running of the Planck mass from ET and CE, respectively. It is clear that a detection of a AGWB in future can open a new window to probe the nature of gravity with good accuracy." @default.
- W3042763725 created "2020-07-23" @default.
- W3042763725 creator A5086929880 @default.
- W3042763725 date "2020-07-23" @default.
- W3042763725 modified "2023-10-17" @default.
- W3042763725 title "Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers" @default.
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- W3042763725 doi "https://doi.org/10.1103/physrevd.102.024071" @default.
- W3042763725 hasPublicationYear "2020" @default.
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