Gravitational radiation observations on the moonThe paper discusses the features of a laser-interferometer gravitational-wave observatory (LIGO) which is planned for operation in the Unitied States, with special attention given to the benefits gained from an addition of a low-mass laser gravitational wave antenna on the moon to the earth-based antennas. It is pointed out that the addition of a moon-based antenna would improve the angular resolution for burst signals by a factor of about 50 (in the plane containing the source, the moon, and the earth), which would be of major importance in studies of gravitational wave sources.
Document ID
19910072003
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Stebbins, R. T. (Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Saulson, P. R. (Joint Institute for Laboratory Astrophysics Boulder, CO, United States)
Armstrong, J. W. (Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Hellings, R. W. (JPL Pasadena, CA, United States)
Bender, P. L. (Joint Institute for Laboratory Astrophysics; NIST, Quantum Physics Div., Boulder CO, United States)
Drever, R. W. P. (California Institute of Technology Pasadena, United States)