All-sky search for high-energy neutrinos from gravitational wave event GW170104 with the ANTARES neutrino telescope

作者：Albert A; Andre M; Anghinolfi M; Anton G; Ardid M; Aubert J J; Avgitas T; Baret B; Barrios Marti J; Basa S; Belhorma B; Bertin V; Biagi S; Bormuth R; Bourret S; Bouwhuis M C; Branza H; Bruijn R; Brunner J; Busto J; Capone A; Caramete L; Carr J; Celli S; El Moursli R Cherkaoui; Chiarusi T; Circella M; Coelho J A B; Coleiro A; Coniglione R; Costantini H; Coyle P; Creusot A; Diaz A F; Deschamps A; De Bonis G; Distefano C; Di Palma I; Domi A; Donzaud C

来源：European Physical Journal C, 2017, 77(12): 911.

DOI：10.1140/epjc/s10052-017-5451-z

Advanced LIGO detected a significant gravitational wave signal (GW170104) originating from the coalescence of two black holes during the second observation run on January 4th, 2017. Anall-sky high-energy neutrino follow-up search has been made using data from the Antares neutrino telescope, including both upgoing and downgoing events in two separate analyses. No neutrino candidates were found within +/- 500 s around the GW event time nor any time clustering of events over an extended time window of +/- 3 months. The non-detection is used to constrain isotropic-equivalent high-energy neutrino emission from GW170104 to less than similar to 1.2 x 10(55) erg for a E-2 spectrum. This constraint is valid in the energy range corresponding to the 5-95% quantiles of the neutrino flux [3.2 TeV; 3.6 PeV], if the GW emitter was below the Antares horizon at the alert time.

• 出版日期2017-12-28