Abstract
In the near future we will witness the coming to a full operational regime of laser interferometers and resonant mass detectors of spherical shape. In this work we study the sensitivity of pairs of such gravitational wave detectors to a scalar stochastic background of gravitational waves. Our computations are carried out both for minimal and nonminimal coupling of the scalar fields.
- Received 9 May 2001
DOI:https://doi.org/10.1103/PhysRevD.64.062001
©2001 American Physical Society
