P010010-00-R - LIGO - California Institute of Technology

List of Tables
xiv
2.1 Comparison of broadband RSE with and without power recycling, as-
suming 10 ppm coating loss. . . . . . . . . . . . . . . . . . . . . . . . 43
2.2 Comparison of broadband RSE with and without power recycling, as-
suming 25 ppm coating loss. . . . . . . . . . . . . . . . . . . . . . . . 43
2.3 1 kHz optimization parameters. . . . . . . . . . . . . . . . . . . . . . 46
2.4 Revised 1 kHz optimization parameters. . . . . . . . . . . . . . . . . 47
2.5 Optical parameters of an interferometer optimized by bench.m for neu-
tron star binary coalescences. . . . . . . . . . . . . . . . . . . . . . . 50
2.6 Power recycled Fabry-Perot Michelson optimization by bench.m for
neutron star binary coalescences. . . . . . . . . . . . . . . . . . . . . 50
2.7 Broadband RSE interferometer optimization by bench.m for neutron
star binary coalescences. . . . . . . . . . . . . . . . . . . . . . . . . . 51
3.1 Matrix of discriminants for an optimized broadband interferometer. . 94
3.2 Variation of phase gains with changing asymmetry. . . . . . . . . . . 95
3.3 Matrix of discriminants for an optimized broadband interferometer,
with optimized asymmetry. . . . . . . . . . . . . . . . . . . . . . . . . 96
3.4 Optical and physical parameters for optimized broadband interferometer. 97
3.5 Common mode residual requirements for the optimized broadband in-
terferometer. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97
3.6 Matrix of discriminants for a 1 kHz narrowband RSE interferometer. 99
3.7 Optical and physical parameters for 1 kHz narrowband interferometer. 99
3.8 Common mode residual requirements for the 1 kHz narrowband inter-
ferometer. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 100
4.1 Calibration of the readout gains of the signal ports. . . . . . . . . . . 112