Optimization of the Euro-Asian network of gravitational detectors for detecting the radiation of collapsing objects
arXiv:2108.12698 · doi:10.1088/1742-6596/2081/1/012011
Abstract
A Euro-Asian network of four gravitational-wave (GW) interferometers is considered, taking into account the plan to create such a detector in Novosibirsk. The efficiency of the network is assessed by typical numerical criteria, which also depend on the characteristics of the received signal. In this work, we calculate the optimal orientation of the Novosibirsk detector for the problem of detecting GW radiation accompanying the collapse of the progenitor star with an initial angular momentum. The specificity of the scenario is the presence of the so-called. bar stage deformation, for which the shape of the emitted GW signal is known.
arXiv admin note: substantial text overlap with arXiv:2009.05860
References in corpus (5)
- Observation of gravitational waves from two neutron star-black hole coalescences
- The gravitational wave burst signal from core collapse of rotating stars
- Localization of gravitational wave sources with networks of advanced detectors
- Global Optimization for Future Gravitational Wave Detectors' Sites
- Interferometer Euro-Asian Network: Detection Characteristics for Signals of Known Shape