Excitation of the modes of a spherical antenna for gravitational waves by high energy particles

Details Excitation of the modes of a spherical antenna for gravitational waves by high energy particles Excitation of the modes of a spherical antenna for gravitational waves by high energy particles

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrvd..64f5017m&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 64, Issue 6, 15 September 2001, id.065017

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Cosmic-Ray Interactions, Gravitational Wave Detectors And Experiments, Thermoelasticity And Electromagnetic Elasticity, Gravitational Radiation Detectors, Mass Spectrometers, And Other Instrumentation And Techniques

Scientific paper

In this paper we determine how the energy generated by the interaction between a high energy particle and a spherical gravitational wave antenna is distributed over the antenna's eigenmodes. We observe that the important mode for gravitational wave detection, the first quadrupole, is much more weakly excited than other modes of interest by this kind of noise.

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