scholarly journals Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

2017 ◽  
Vol 96 (2) ◽  
Author(s):  
A. Albert ◽  
M. André ◽  
M. Anghinolfi ◽  
G. Anton ◽  
M. Ardid ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
High Energy ◽  
Wave Event ◽  
High Energy Neutrinos

scholarly journals High-energy neutrinos from the gravitational wave event GW150914 possibly associated with a short gamma-ray burst

2016 ◽  
Vol 93 (12) ◽  
Author(s):  
Reetanjali Moharana ◽  
Soebur Razzaque ◽  
Nayantara Gupta ◽  
Peter Mészáros
Keyword(s):  
Gravitational Wave ◽  
Gamma Ray ◽  
High Energy ◽  
Gamma Ray Burst ◽  
Wave Event ◽  
High Energy Neutrinos

scholarly journals Multi-messenger searches via IceCube’s high-energy neutrinos and gravitational-wave detections of LIGO/Virgo

2021 ◽  
Author(s):  
Doğa Veske ◽  
Rasha Abbasi ◽  
Markus Ackermann ◽  
Jenni Adams ◽  
Juanan Aguilar ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
High Energy ◽  
High Energy Neutrinos

JOINT SEARCHES BETWEEN GRAVITATIONAL-WAVE INTERFEROMETERS AND HIGH-ENERGY NEUTRINO TELESCOPES: SCIENCE REACH AND ANALYSIS STRATEGIES

2009 ◽  
Vol 18 (10) ◽  
pp. 1655-1659 ◽  
Author(s):  
VERONIQUE VAN ELEWYCK ◽  
S. ANDO ◽  
Y. ASO ◽  
B. BARET ◽  
M. BARSUGLIA ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Gravitational Waves ◽  
High Energy ◽  
Directional Information ◽  
High Energy Neutrino ◽  
Neutrino Telescopes ◽  
Energy Neutrino ◽  
Analysis Strategies ◽  
High Energy Neutrinos

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.

scholarly journals Neutrino fluence from gamma-ray bursts: off-axis view of structured jets

2019 ◽  
Vol 490 (4) ◽  
pp. 4935-4943 ◽  
Author(s):  
Markus Ahlers ◽  
Lea Halser
Keyword(s):  
Gravitational Wave ◽  
Angular Dependence ◽  
Gamma Rays ◽  
Gamma Ray ◽  
High Energy ◽  
Gamma Ray Bursts ◽  
Scaling Relation ◽  
Model Predictions ◽  
Wave Event ◽  
Axis View

ABSTRACT We investigate the expected high-energy neutrino fluence from internal shocks produced in the relativistic outflow of gamma-ray bursts. Previous model predictions have primarily focused on on-axis observations of uniform jets. Here, we present a generalization to account for arbitrary viewing angles and jet structures. Based on this formalism, we provide an improved scaling relation that expresses off-axis neutrino fluences in terms of on-axis model predictions. We also find that the neutrino fluence from structured jets can exhibit a strong angular dependence relative to that of gamma-rays and can be far more extended. We examine this behaviour in detail for the recent short gamma-ray burst GRB 170817A observed in coincidence with the gravitational wave event GW170817.

scholarly journals Gravitational-wave follow-up with CTA after the detection of GRBs in the TeV energy domain

2019 ◽  
Vol 490 (3) ◽  
pp. 3476-3482 ◽  
Author(s):  
I Bartos ◽  
K R Corley ◽  
N Gupte ◽  
N Ash ◽  
Z Márka ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Gamma Ray ◽  
The United States ◽  
High Energy ◽  
Cherenkov Telescopes ◽  
Wave Event ◽  
Energy Domain ◽  
Time Requirements ◽  
High Energy Emission

ABSTRACT The recent discovery of TeV emission from gamma-ray bursts (GRBs) by the MAGIC and H.E.S.S. Cherenkov telescopes confirmed that emission from these transients can extend to very high energies. The TeV energy domain reaches the most sensitive band of the Cherenkov Telescope Array (CTA). This newly anticipated, improved sensitivity will enhance the prospects of gravitational-wave follow-up observations by CTA to probe particle acceleration and high-energy emission from binary black hole and neutron star mergers, and stellar core-collapse events. Here we discuss the implications of TeV emission on the most promising strategies of choice for the gravitational-wave follow-up effort for CTA and Cherenkov telescopes more broadly. We find that TeV emission (i) may allow more than an hour of delay between the gravitational-wave event and the start of CTA observations; (ii) enables the use of CTA’s small size telescopes that have the largest field of view. We characterize the number of pointings needed to find a counterpart. (iii) We compute the annual follow-up time requirements and find that prioritization will be needed. (iv) Even a few telescopes could detect sufficiently nearby counterparts, raising the possibility of adding a handful of small-sized or medium-sized telescopes to the network at diverse geographic locations. (v) The continued operation of VERITAS/H.E.S.S./MAGIC would be a useful compliment to CTA’s follow-up capabilities by increasing the sky area that can be rapidly covered, especially in the United States and Australia, in which the present network of gravitational-wave detectors is more sensitive.

scholarly journals High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube

2016 ◽  
Vol 93 (12) ◽  
Author(s):  
S. Adrián-Martínez ◽  
A. Albert ◽  
M. André ◽  
M. Anghinolfi ◽  
G. Anton ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino ◽  
Wave Event

scholarly journals Bounding the time delay between high-energy neutrinos and gravitational-wave transients from gamma-ray bursts

2011 ◽  
Vol 35 (1) ◽  
pp. 1-7 ◽  
Author(s):  
Bruny Baret ◽  
Imre Bartos ◽  
Boutayeb Bouhou ◽  
Alessandra Corsi ◽  
Irene Di Palma ◽  
...  
Keyword(s):  
Time Delay ◽  
Gravitational Wave ◽  
Gamma Ray ◽  
High Energy ◽  
Gamma Ray Bursts ◽  
High Energy Neutrinos
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