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LISA, binary stars, and the mass of the graviton
Curt Cutler, William A. Hiscock, Shane L. Larson
We extend and improve earlier estimates of the ability of the proposed LISA (Laser Interferometer Space Antenna) gravitational wave detector to place upper bounds on the graviton m…
The LISA Optimal Sensitivity
Thomas A. Prince, Massimo Tinto, Shane L. Larson +1
The multiple Doppler readouts available on the Laser Interferometer Space Antenna (LISA) permit simultaneous formation of several interferometric observables. All these observables…
Unequal arm space-borne gravitational wave detectors
Shane L. Larson, Ronald W. Hellings, William A. Hiscock
Unlike ground-based interferometric gravitational wave detectors, large space-based systems will not be rigid structures. When the end-stations of the laser interferometer are free…
LISA data analysis I: Doppler demodulation
Neil Cornish, Shane Larson
The orbital motion of the Laser Interferometer Space Antenna (LISA) produces amplitude, phase and frequency modulation of a gravitational wave signal. The modulations have the effe…