Excluding Source Models with Multiple Astrophysical Observations
arXiv:1303.1549
Abstract
We describe a general method to observationally exclude a theoretical model for gravitational wave (GW) emission from a transient astrophysical source (event) by using a null detection from a network of GW detectors. In the case of multiple astrophysical events with no GW detection, statements about individual events can be combined to increase the exclusion confidence. We frame and demonstrate the method using a population of hypothetical core collapse supernovae.
arXiv comment10 pages, 5 figures
References in corpus (5)
- A Unified Approach to the Classical Statistical Analysis of Small Signals
- Search for Gravitational Wave Bursts from Soft Gamma Repeaters
- Search for Gravitational Wave Bursts from Six Magnetars
- Stacked Search for Gravitational Waves from the 2006 SGR 1900+14 Storm
- Search for Gravitational Waves Associated with 39 Gamma-Ray Bursts Using Data from the Second, Third, and Fourth LIGO Runs