Mid-Frequency Gravitational Wave Detection and Sources
General Relativity and Quantum Cosmology
2020-07-14 v2 Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
Abstract
A brief history and various themes of mid-frequency gravitational wave detection are presented more or less following historical order -- Laser Interferometry, Atom Interferometry (AI), Torsion Bar Antenna (TOBA), and Superconducting Omni-directional Gravitational Radiation Observatory (SOGRO). Both Earth-based and Space-borne concepts are reviewed with outlook on expected astrophysical sources
Cite
@article{arxiv.2004.05590,
title = {Mid-Frequency Gravitational Wave Detection and Sources},
author = {Wei-Tou Ni},
journal= {arXiv preprint arXiv:2004.05590},
year = {2020}
}
Comments
reference update and minor corrections