Response of spherical gravitational wave antenna modes to high-energy cosmic ray particles

Details Response of spherical gravitational wave antenna modes to high-energy cosmic ray particles Response of spherical gravitational wave antenna modes to high-energy cosmic ray particles

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cqgra..19.1955m&link_type=abstract

Classical and Quantum Gravity, Volume 19, Issue 7, pp. 1955-1960 (2002).

Physics

Scientific paper

High-energy cosmic ray particles are expected to be a significant source of noise in resonant mass gravitational wave detectors close to the quantum limit. The spherical, fourth generation antennas have been designed to attain such a limit. In this work we will show how the energy of a cosmic ray particle interacting with such an antenna is distributed over its eigenmodes. We will then make some comments on the relevant consequences of such a distribution for gravitational wave detection.

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