LIGO Document P1000041-v1
- We derive a simple relationship between the energy emitted in gravitational waves for a narrowband source and the distance to which that emission can be detected by a single detector. We consider both linearly polarized and elliptically polarized gravitational waves. We also consider several emission patterns: isotropic emission (unrealistic but simple), and emission patterns appropriate for sources that emit linearly or circularly polarized waves. We ignore cosmological effects.
DCC Version 3.5.0, contact
DCC Help