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Multimessenger Sources of Gravitational Waves and High-energy Neutrinos: Science Reach and Analysis Method

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons1448

Di Palma,  I.
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons60743

Papa,  M. A.
Laser Physics, Max Planck Institute of Quantum Optics, Max Planck Society;

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JoPCS_363_1_012022.pdf
(beliebiger Volltext), 2MB

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Zitation

Baret, B., Bartos, I., Bouhou, B., Chassande-Mottin, E., Corsi, A., Di Palma, I., et al. (2012). Multimessenger Sources of Gravitational Waves and High-energy Neutrinos: Science Reach and Analysis Method. Journal of Physics: Conference Series, 363(1): 012022. doi:10.1088/1742-6596/363/1/012022.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000E-7CDC-6
Zusammenfassung
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 with a gravitational-wave signal could be a crucial aspect for the first direct detection of gravitational waves. Furthermore, combining gravitational waves with electromagnetic and neutrino observations will enable the extraction of scientific insight that was hidden from us before. We discuss the method that enables the joint search with the LIGO-Virgo-IceCube-ANTARES global network, as well as its methodology, science reach, and outlook for the next generation of gravitational-wave detectors.