Fast radio bursts (FRBs), millisecond-duration bursts prevailing in the radio sky, are the
latest large puzzle in the Universe and have been a subject of intense observational and …

Gravitational-wave detections are enabling measurements of the rate of coalescences of
binaries composed of two compact objects—neutron stars and/or black holes. The …

Now that detection of gravitational-wave signals from the coalescence of extra-galactic
compact binary star mergers has become nearly routine, it is intriguing to consider other …

Combining the GW observations of merging systems of binary neutron stars and quasi-
universal relations, we set constraints on the maximum mass that can be attained by …

At present, we have almost as many theories to explain Fast Radio Bursts as we have Fast
Radio Bursts observed. This landscape will be changing rapidly with CHIME/FRB, recently …

The first observation of a binary neutron star (NS) coalescence by the Advanced LIGO and
Advanced Virgo gravitational-wave (GW) detectors offers an unprecedented opportunity to …

In a single process, the merger of binary neutron star systems combines extreme gravity, the
copious emission of gravitational waves, complex microphysics and electromagnetic …

In this article, I introduce ideas and techniques to extract information about the equation of
state of matter at very high densities from gravitational waves emitted before, during and …

With the first observation of a binary neutron star merger through gravitational waves and
light, GW170817, compact binary mergers have now taken the center stage in nuclear …

On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors
observed a low-mass compact binary inspiral. The initial sky localization of the source of the …