Mid-Frequency Gravitational Waves (0.1-10 Hz): Sources and Detection Methods Summary of the parallel session GW2 of MG16 Meeting
arXiv:2111.09715
Abstract
This article summarizes the talks in the session GW2 of the Sixteenth Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation, and Relativistic Field Theories, 5-10 July, 2021, on Mid-frequency (0.1-10 Hz) gravitational waves: Sources and detection methods with a review on strain power spectral density amplitude of various mid-frequency gravitational wave projects/concepts and with extended summaries on the progress of ZAIGA project and on the conceptual study of AMIGO.
arXiv comment16 pages, 3 figures, 1 table
References in corpus (13)
- The promise of multi-band gravitational wave astronomy
- AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space
- A Horizon Study for Cosmic Explorer: Science, Observatories, and Community
- ZAIGA: Zhaoshan Long-baseline Atom Interferometer Gravitation Antenna
- Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
- The astrophysical science case for a decihertz gravitational-wave detector
- Prospects of determination of reheating temperature after inflation by DECIGO
- Gravitational-Wave Lunar Observatory for Cosmology
- United test of the equivalence principle at level using mass and internal energy specified atoms
- Direct determination of supermassive black hole properties with gravitational-wave radiation from surrounding stellar-mass black hole binaries
- LISA Pathfinder Performance Confirmed in an Open-Loop Configuration: Results from the Free-Fall Actuation Mode
- Gravitational wave cosmology I: high frequency approximation
- Ultralight scalar dark matter detection with ZAIGA