Geometry of transient gravitational waves and estimation of efficiencies of different detector configurations
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.
Authors
- Osvaldo M. Moreschi (ORCID: https://orcid.org/0000-0001-9753-3820)
Institutions
- Universidad Nacional de Córdoba (AR)
Publication Details
- Journal
- International Journal of Geometric Methods in Modern Physics
- Published
- 2026-04-30
- DOI
- https://doi.org/10.1142/s021988782650221x
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00