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Snowmass2021 Cosmic Frontier White Paper: Future Gravitational-Wave Detector Facilities

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arxiv 2203.08228 v2 pith:4EEY4D6J submitted 2022-03-15 gr-qc astro-ph.IMhep-exhep-th

Stefan W. Ballmer , Rana Adhikari , Leonardo Badurina , Duncan A. Brown , Swapan Chattopadhyay , Matthew Evans , Peter Fritschel , Evan Hall
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Jason M. Hogan Karan Jani Tim Kovachy Kevin Kuns Ariel Schwartzman Daniel Sigg Bram Slagmolen Salvatore Vitale Christopher Wipf
This is my paper · ORCID
classification gr-qcastro-ph.IMhep-exhep-th
keywords gravitational-wavecosmicdetectoruniversefuturehistoryinteractionmatter
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The next generation of gravitational-wave observatories can explore a wide range of fundamental physics phenomena throughout the history of the universe. These phenomena include access to the universe's binary black hole population throughout cosmic time, to the universe's expansion history independent of the cosmic distance ladders, to stochastic gravitational-waves from early-universe phase transitions, to warped space-time in the strong-field and high-velocity limit, to the equation of state of nuclear matter at neutron star and post-merger densities, and to dark matter candidates through their interaction in extreme astrophysical environments or their interaction with the detector itself. We present the gravitational-wave detector concepts than can drive the future of gravitational-wave astrophysics. We summarize the status of the necessary technology, and the research needed to be able to build these observatories in the 2030s.

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Cited by 2 Pith papers

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  1. Conservative Black Hole Scattering at Fifth Post-Minkowskian and Second Self-Force Order

    hep-th 2026-01 conditional novelty 7.0 of 10

    The conservative black-hole scattering angle at fifth post-Minkowskian and second self-force order is computed in terms of K3 periods, but contains a coefficient fixed only by an ad hoc 'γ-3' prescription.

  2. Birefringence in fermion-attenuated gravitational wave power spectrum

    gr-qc 2025-01 conditional novelty 5.0 of 10

    Combining free-streaming fermion damping with Chern-Simons gravity yields a chiral asymmetry and oscillatory peaks and dips in the stochastic gravitational wave power spectrum.

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