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

2012 ◽  
Vol 363 ◽  
pp. 012022 ◽  
Author(s):  
B Baret ◽  
I Bartos ◽  
B Bouhou ◽  
E Chassande-Mottin ◽  
A Corsi ◽  
...  
2012 ◽  
Vol 85 (10) ◽  
Author(s):  
Bruny Baret ◽  
Imre Bartos ◽  
Boutayeb Bouhou ◽  
Eric Chassande-Mottin ◽  
Alessandra Corsi ◽  
...  

2010 ◽  
Vol 243 ◽  
pp. 012002 ◽  
Author(s):  
Eric Chassande-Mottin ◽  
the Ligo Scientific Collaboration a Collaboration

2014 ◽  
Vol 90 (10) ◽  
Author(s):  
M. G. Aartsen ◽  
M. Ackermann ◽  
J. Adams ◽  
J. A. Aguilar ◽  
M. Ahlers ◽  
...  

2009 ◽  
Vol 18 (10) ◽  
pp. 1655-1659 ◽  
Author(s):  
VERONIQUE VAN ELEWYCK ◽  
S. ANDO ◽  
Y. ASO ◽  
B. BARET ◽  
M. BARSUGLIA ◽  
...  

Many of the astrophysical sources and violent phenomena observed in our Universe are potential emitters of gravitational waves (GWs) and high-energy neutrinos (HENs). A network of GW detectors such as LIGO and Virgo can determine the direction/time of GW bursts while the IceCube and ANTARES neutrino telescopes can also provide accurate directional information for HEN events. Requiring the consistency between both, totally independent, detection channels shall enable new searches for cosmic events arriving from potential common sources, of which many extra-galactic objects.


2013 ◽  
Vol 2013 (06) ◽  
pp. 008-008 ◽  
Author(s):  
S Adrián-Martínez ◽  
I. Al Samarai ◽  
A Albert ◽  
M André ◽  
M Anghinolfi ◽  
...  

2019 ◽  
Vol 207 ◽  
pp. 02010 ◽  
Author(s):  
Lisa Schumacher

The IceCube Neutrino Observatory has recently found compelling evidence for a particular blazar producing high-energy neutrinos and PeV cosmic rays, however the sources of cosmic rays above several EeV remain unidentified. It is believed that the same environments that accelerate ultra-high-energy cosmic rays (UHECRs) also produce high-energy neutrinos via hadronic interactions of lower-energy cosmic rays. Two out of three joint analyses of the Ice- Cube Neutrino Observatory, the Pierre Auger Observatory and the Telescope Array yielded hints for a possible directional correlation of high-energy neutrinos and UHECRs. These hints however became less significant with more data. Recently, an improved analysis with an approach complementary to the other analyses has been developed. This analysis searches for neutrino point sources in the vicinity of UHECRs with search windows estimated from deflections by galactic magnetic fields. We present this new analysis method for searching common hadronic sources, additionally including neutrino data measured by ANTARES in order to increase the sensitivity to possible correlations in the Southern Hemisphere.


2019 ◽  
Vol 100 (8) ◽  
Author(s):  
Imre Bartos ◽  
Doğa Veske ◽  
Azadeh Keivani ◽  
Zsuzsa Márka ◽  
Stefan Countryman ◽  
...  

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