MG13 - Talk detail |
Participant |
Bartos, Imre | |||||||
Institution |
Columbia University - 538 West 120th Street - New York - NY - USA | |||||||
Session |
GW2 |
Accepted |
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Order |
Time |
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Talk |
Oral abstract |
Title |
Gravitational Wave and High Energy Neutrino Multimessenger Searches: Probing the Population and Structure of Jet Driven Core-Collapse Supernova and Long Gamma Ray Burst Progenitors | |||||
Co-authors | ||||||||
Abstract |
Sources of gravitational waves are often expected to be observable through several messengers, such as gamma-rays, X-rays, optical, radio, and/or neutrino emission. The simultaneous observation of electromagnetic or neutrino emission could be a crucial aspect for the first direct detection of gravitational waves. Information on the progenitor, such as trigger time, direction and expected frequency range, can enhance our ability to identify gravitational wave signatures with amplitudes close to the noise floor of the detector. Furthermore, combining gravitational waves with electromagnetic and neutrino observations will enable the extraction of scientific insight that was hidden from us before. We discuss recent development and plans in searches for common sources with the IceCube-ANTARES-LIGO-GEO-Virgo global network as well as their methodology, science reach, and outlook for next generation gravitational-wave detectors. |
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