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Report of the Topical Group on Cosmic Probes of Fundamental Physics for for Snowmass 2021
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Cosmic Probes of Fundamental Physics take two primary forms: Very high energy particles (cosmic rays, neutrinos, and gamma rays) and gravitational waves. Already today, these probes give access to fundamental physics not available by any other means, helping elucidate the underlying theory that completes the Standard Model. The last decade has witnessed a revolution of exciting discoveries such as the detection of high-energy neutrinos and gravitational waves. The scope for major developments in the next decades is dramatic, as we detail in this report.
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Cited by 2 Pith papers
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The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
The gravitational wave bias of mock binary black holes increases with the pivot mass of the assumed host galaxy mass selection, and can exceed the galaxy bias by up to about 30 percent only for steep host probability slopes.
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UHECR measurements and physics at man-made accelerators: mutual constraints
A review of the mutual constraints between UHECR air-shower observations and accelerator measurements, centered on the muon puzzle and future experimental tests.
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