Decihertz (~0.1 Hz) Gravitational Wave Detection
There are an exceptionally large number of compelling signals that live in this band, including: the elusive intermediate mass black holes, white dwarf mergers (putative SN Ia progenitor), tidal disruption events, high precession and eccentricity systems, neutron star merger early warning, and more.
Resources (1)
R&D Gaps (1)
Detecting gravitational waves allows us to observe cosmic events like black hole mergers and neutron star collisions that are invisible through traditional telescopes. Current gravitational wave detectors are primarily sensitive to audio-band signals. Some phenomena, including speculative ones such ...