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  Multimessenger astrophysics: When gravitational waves meet high energy neutrinos

Di Palma, I., ANTARES Collaboration, LIGO Sci Collaboration, & VIRGO Collaboration (2014). Multimessenger astrophysics: When gravitational waves meet high energy neutrinos. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 742, 124-129. doi:10.1016/j.nima.2013.10.076.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-001A-0D4D-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-001A-0D4F-1
Genre: Journal Article

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Di Palma, Irene1, Author              
ANTARES Collaboration , Author              
LIGO Sci Collaboration, Author              
VIRGO Collaboration , Author              
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1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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 Abstract: With recent development of experimental techniques that have opened new windows of observation of the cosmic radiation in all its components, multi-messenger astronomy is entering an exciting era. Many astrophysical sources and cataclysmic cosmic events with burst activity can be plausible sources of concomitant gravitational waves (GWs) and high-energy neutrinos (HENS). Such messengers could reveal hidden and new sources that are not observed by conventional photon astronomy, in particular at high energy. Requiring consistency between GW and HEN detection channels enables new searches and a detection would yield significant additional information about the common source. We present the results of the first search for gravitational wave bursts associated with high energy neutrino triggers, detected by the underwater neutrino telescope ANTARES in its 5 line configuration, during the fifth LIGO science run and first Virgo science run. No evidence for coincident events was found. We place a lower limit on the distance to GW sources associated with every HEN trigger. We are able to rule out the existence of coalescing binary neutron star systems and black hole-neutron star systems up to distances that are typically 5 Mpc and 10 Mpc respectively.

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 Dates: 2014
 Publication Status: Published in print
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 Identifiers: DOI: 10.1016/j.nima.2013.10.076
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Title: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Source Genre: Journal
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Pages: - Volume / Issue: 742 Sequence Number: - Start / End Page: 124 - 129 Identifier: -