GW4 - Middle-Frequency (0.1 Hz to 10 Hz) Gravitational Wave (GW) Detection and its Sources |
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Speaker |
Ni, Wei-Tou |
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| Talk Title |
Middle-Frequency (0.1 Hz to 10 Hz) GW Detection and its Sources: An Overview |
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Abstract |
With the detection of high-frequency GWs from the coalescence of stellar-size black holes and neutron stars, we are formally ushered into the age of gravitational-wave astronomy. LISA Pathfinder (LPF) launched on 3 December 2015 has completely met the stringent LISA drag-free demand and has successfully paves the road for space detection of low frequency (0.1 Hz to 0.1 Hz) GWs and middle-frequency (0.1 Hz to 10 Hz) GWs. Talks will be focused on recent activities both for Earth-based and space borne detection of middle-frequency GWs: GW sources, Newtonian Noise Cancellation, TOBA (Torsion Bar Antenna), MIGA (Matter-wave laser Interferometric Gravitation Antenna), AIGSO (Atomic Interferometric Gravitational-wave Space Observatory), MAGIS (Mid-band Atomic Gravitational Wave Interferometric Sensor), AMIGO (Astrodynamical Middle-Frequency Interferometric Gravitational-wave Observatory), SOGRO (Superconducting Omni-directioanl Gravitational Radiation Observatory), etc. This talk is an overview of this session. |
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