Resonance method of geophysical signal detection by laser gravitational antennas

A.V. Gusev, V.N. Rudenko, I.S. Yudin1


We consider the role of an additional mirror (recycling) in the design of long-base gravitational wave laser interferometers for the detection of weak infra-low-frequency geophysical signals by the resonance method


  1. A. V. Gusev and V. N. Rudenko, Gravitational modulation of the optical length of long-base πe laser interferometers. JETP letters 91(10), 543 (2010)
  2. A. V. Gusev, V. N. Rudenko, and I. S. Yudin, Detection of slow geophysical perturbations with gravitationalwave interferometers. Izmeritel'naya Tekhnika No. 6 (2011).
  3. A. V. Gusev and I. S. Yudin, A locally optimal algorithm for finding weak geophysical signals at the output of laser gravitational antennas. Vestnik Mosk. Univ., Series 3: Physics, Astronomy. No. 2 (2012).
  4. A. V. Gusev, V. N. Rudenko, and I. S. Yudin, Laser interferometric gravitational antennas: the role of recycling in the "free spectrum range" regime. Izmeritel'naya Tekhnika No. 4 (2012).
  5. A. V. Gusev, V. N. Rudenko, and I. S. Yudin, A new scheme of geophysical signal detection with optical gravitational antennas. Grav. Cosmol. 18(2) (2012).
  6. A. V. Gusev and V. N. Rudenko, Geophysical noise of VIRGO gravitational antenna. Izmeritel'naya Tekhnika No. 2, 3 (2009).
  7. B. P. Abbott et al., LIGO: the Laser Interferometer Gravitational-Wave Observatory. Rep. Prog. Phys. 72, 076901 (2009).
  8. P. Acernese et al., Status of Virgo, Class. Quantum Grav. 25, 114045 (2008).
For more information about this paper please visit Springer's Home Page of this paper.

Back to The Contents Page