Spinning neutron stars (NSs) can emit continuous gravitational waves (GWs) that carry a
wealth of information about the compact object. If such a signal is detected, it will provide us …

Neutron star (NS) binaries can be potentially intriguing gravitational wave sources, with both
high-and low-frequency radiation from the possibly aspherical individual stars and the …

LIGO and Virgo recently made the first observation of a binary neutron star merger
demonstrating that gravitational-wave observations offer the ability to probe how matter …

We construct an efficient frequency domain waveform for generic circular compact object
binaries that include neutron stars. The orbital precession is solved on the radiation reaction …

We study gravitational wave searches for merging binary neutron stars (NSs). We use
nonspinning template waveforms towards the signals emitted from aligned-spin NS-NS …

The parameters of inspiraling compact binaries can be estimated using matched filtering of
gravitational-waveform templates against the output of laser-interferometric gravitational …

Gravitational waves (GWs) from binary neutron stars (NSs) have opened unique
opportunities to constrain the nuclear equation of state by measuring tidal effects associated …

Inspiraling binary neutron stars (BNSs) are expected to be one of the most significant
sources of gravitational-wave signals for the new generation of advanced ground-based …

We study the orbital evolution of eccentric binary neutron stars. The motion follows a quasi-
Keplarian orbit with perturbations due to tidal couplings. We find that the tidal interaction …

The precise measurement of neutron star (NS) spins can provide important insight into the
formation and evolution of compact binaries containing NS. While traditional methods of NS …