High-energy multimessenger transient astrophysics
The recent discoveries of high-energy cosmic neutrinos and gravitational waves from
astrophysical objects have led to a new era of multimessenger astrophysics. In particular …
astrophysical objects have led to a new era of multimessenger astrophysics. In particular …
The delay time of gravitational wave—gamma-ray burst associations
B Zhang - Frontiers of Physics, 2019 - Springer
The first gravitational wave (GW)—gamma-ray burst (GRB) association, GW170817/GRB
170817A, had an offset in time, with the GRB trigger time delayed by∼ 1.7 s with respect to …
170817A, had an offset in time, with the GRB trigger time delayed by∼ 1.7 s with respect to …
High-energy neutrino emission from short gamma-ray bursts: prospects for coincident detection with gravitational waves
We investigate current and future prospects for coincident detection of high-energy neutrinos
and gravitational waves (GWs). Short gamma-ray bursts (SGRBs) are believed to originate …
and gravitational waves (GWs). Short gamma-ray bursts (SGRBs) are believed to originate …
Electromagnetic signals following stellar-mass black hole mergers
SE De Mink, A King - The Astrophysical Journal Letters, 2017 - iopscience.iop.org
It is often assumed that gravitational-wave (GW) events resulting from the merger of stellar-
mass black holes are unlikely to produce electromagnetic (EM) counterparts. We point out …
mass black holes are unlikely to produce electromagnetic (EM) counterparts. We point out …
Can an off-axis gamma-ray burst jet in GW170817 explain all the electromagnetic counterparts?
K Ioka, T Nakamura - Progress of Theoretical and Experimental …, 2018 - academic.oup.com
Gravitational waves from a merger of two neutron stars (NSs) were discovered for the first
time in GW170817, together with diverse electromagnetic (EM) counterparts. To make …
time in GW170817, together with diverse electromagnetic (EM) counterparts. To make …
Search for multimessenger sources of gravitational waves and high-energy neutrinos with advanced LIGO during its first observing run, ANTARES, and IceCube
We have entered the era of regular gravitational-wave (GW) discoveries. Since 2015,
Advanced LIGO (Abadie et al. 2015) and Advanced Virgo (Acernese et al. 2015) have …
Advanced LIGO (Abadie et al. 2015) and Advanced Virgo (Acernese et al. 2015) have …
GW 150914-like black holes as Galactic high-energy sources
K Ioka, T Matsumoto, Y Teraki… - Monthly Notices of …, 2017 - academic.oup.com
The first direct detections of gravitational waves (GWs) from black hole (BH) mergers, GW
150914, GW 151226 and LVT 151012, give a robust lower limit on the number of merged …
150914, GW 151226 and LVT 151012, give a robust lower limit on the number of merged …
Single progenitor model for GW150914 and GW170104
DJ D'Orazio, A Loeb - Physical Review D, 2018 - APS
The merger of stellar-mass black holes (BHs) is not expected to generate detectable
electromagnetic (EM) emission. However, the gravitational wave (GW) events GW150914 …
electromagnetic (EM) emission. However, the gravitational wave (GW) events GW150914 …
Charged compact binary coalescence signal and electromagnetic counterpart of plunging black hole–neutron star mergers
B Zhang - The Astrophysical Journal Letters, 2019 - iopscience.iop.org
If at least one of the members of a compact binary coalescence is charged, the inspiral of the
two members would generate a Poynting flux with an increasing power, giving rise to a brief …
two members would generate a Poynting flux with an increasing power, giving rise to a brief …
[PDF][PDF] Energetic constraints on electromagnetic signals from double black hole mergers
The possible Fermi detection of an electromagnetic counterpart to the double black hole
merger GW150914 has inspired many theoretical models, some of which propose that the …
merger GW150914 has inspired many theoretical models, some of which propose that the …