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- W2904557327 abstract "A primordial spectrum of gravitational waves serves as a backlight to the relativistic degrees of freedom of the cosmological fluid. Any change in the particle physics content, due to a change of phase or freeze-out of a species, will leave a characteristic imprint on an otherwise featureless primordial spectrum of gravitational waves and indicate its early-Universe provenance. We show that a gravitational wave detector such as the Laser Interferometer Space Antenna would be sensitive to physics near 100 TeV in the presence of a sufficiently strong primordial spectrum. Such a detection could complement searches at newly proposed 100 km circumference accelerators such as the Future Circular Collider at CERN and the Super Proton-Proton Collider in China, thereby providing insight into a host of beyond standard model issues, including the hierarchy problem, dark matter, and baryogenesis." @default.
- W2904557327 created "2018-12-22" @default.
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- W2904557327 date "2019-08-06" @default.
- W2904557327 modified "2023-10-15" @default.
- W2904557327 title "Using a primordial gravitational wave background to illuminate new physics" @default.
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- W2904557327 doi "https://doi.org/10.1103/physrevd.100.043513" @default.
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