Interferometers for displacement-noise-free gravitational-wave detection.
We propose a class of displacement- and laser-noise-free gravitational-wave-interferometer configurations, which does not sense nongeodesic mirror motion and laser noise, but provides a nonvanishing gravitational-wave signal. Our interferometers consist of four mirrors and two beam splitters, which form four Mach-Zehnder interferometers. By contrast to previous works, no composite mirrors with multiple reflective surfaces are required. Each mirror in our configuration is sensed redundantly, by at least two pairs of incident and reflected beams. Displacement- and laser-noise-free detection is achieved when output signals from these four interferometers are combined appropriately. Our 3-dimensional interferometer configuration has a low-frequency response proportional to f2, which is better than the f3 achievable by previous 2-dimensional configurations.
Chen
Yanbei
Y
Max-Planck Institut für Gravitationsphysik, Am Mühlenberg 1, 14476 Potsdam, Germany.
Pai
Archana
A
Somiya
Kentaro
K
Kawamura
Seiji
S
Sato
Shuichi
S
Kokeyama
Keiko
K
Ward
Robert L
RL
Goda
Keisuke
K
Mikhailov
Eugeniy E
EE