Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory

A Aab, P Abreu, M Aglietta, I Al Samarai… - Physical Review D, 2016 - APS
On September 14, 2015 the Advanced LIGO detectors observed their first gravitational wave
(GW) transient GW150914. This was followed by a second GW event observed on
December 26, 2015. Both events were inferred to have arisen from the merger of black holes
in binary systems. Such a system may emit neutrinos if there are magnetic fields and disk
debris remaining from the formation of the two black holes. With the surface detector array of
the Pierre Auger Observatory we can search for neutrinos with energy E ν above 100 PeV …

Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory

F Arqueros Martínez, D García Pinto, IA Minaya Flores… - 2016 - docta.ucm.es
On September 14, 2015 at 09∶ 50∶ 45 universal time (UTC) the Advanced LIGO detectors
observed the first gravitational wave (GW) transient GW150914 [1]. The GW was inferred to
have arisen from the merger of black holes in a binary system at a luminosity distance Ds=
410+ 160− 180 Mpc. The estimated amount of energy released in the form of gravitational
waves was EGW= 3.0+ 0.5− 0.5 M⊙ c 2 solar masses [1, 2]. A second GW event GW151226
[3] was detected at 03∶ 38∶ 53 UTC on December 26, 2015, also inferred to be produced …
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