Geometry of transient gravitational waves and estimation of efficiencies of different detector configurations
arXiv:2604.24433 · doi:10.1142/S021988782650221X
Abstract
This work introduces a geometrical method for analyzing transient gravitational waves recorded at interferometric observatories. This approach is intended to aid in assessing the performance and sensitivity of next-generation detector configurations, such as Cosmic Explorer, Einstein Telescope, and the South American Gravitational-wave Observatory.
14 pages. Accepted for publication in Int. J. Geom. Meth. Mod. Phys