Multimessenger Sources of Gravitational Waves and High-energy Neutrinos: Science Reach and Analysis Method
Bruny Baret
(1)
,
Imre Bartos
(2)
,
Boutayeb Bouhou
(1)
,
Eric Chassande-Mottin
(1)
,
Alessandra Corsi
(3)
,
Irene Di Palma
(4)
,
Corinne Donzaud
(1, 5)
,
Marco Drago
(6)
,
Chad Finley
(7)
,
Geraint H. Jones
(8)
,
Sergey Klimenko
(9)
,
Antoine Kouchner
(1)
,
Szabolcs Márka
(2)
,
Zsuzsa Márka
(2)
,
Luciano Moscoso
(1)
,
M. Alessandra Papa
(4)
,
Thierry Pradier
(10)
,
Giovanni Prodi
(6)
,
Peter Raffai
(2)
,
Virginia Re
(11)
,
J. Rollins
(3)
,
Francesco Salemi
(4)
,
Patrick J. Sutton
(8)
,
Maggie Tse
(2)
,
Véronique van Elewyck
(1)
,
Gabriele Vedovato
(12)
1
APC (UMR_7164) -
AstroParticule et Cosmologie
2 Department of Physics, Columbia University
3 LIGO - Laser Interferometer Gravitational-Wave Observatory
4 Max-Planck-Institut für Gravitationsphysik
5 UP11 - Université Paris-Sud - Paris 11
6 INFN - Gruppo Collegato di Trento
7 Oskar Klein Centre, Physics Department
8 Cardiff University
9 University of Florida
10 IPHC - Institut Pluridisciplinaire Hubert Curien
11 INFN - Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata
12 INFN - Istituto Nazionale di Fisica Nucleare, Sezione di Padova
2 Department of Physics, Columbia University
3 LIGO - Laser Interferometer Gravitational-Wave Observatory
4 Max-Planck-Institut für Gravitationsphysik
5 UP11 - Université Paris-Sud - Paris 11
6 INFN - Gruppo Collegato di Trento
7 Oskar Klein Centre, Physics Department
8 Cardiff University
9 University of Florida
10 IPHC - Institut Pluridisciplinaire Hubert Curien
11 INFN - Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata
12 INFN - Istituto Nazionale di Fisica Nucleare, Sezione di Padova
Résumé
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.