Gravitational waves emitted from the coalescence of neutron star binaries open a new
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …

Gravitational waves from neutron star binary inspirals contain information on strongly
interacting matter in unexplored, extreme regimes. Extracting this requires robust theoretical …

The deformability of a compact object under the presence of a tidal perturbation is encoded
in the tidal Love numbers (TLNs), which vanish for isolated black holes in vacuum. We show …

Gravitational-wave astronomy with coalescing binary neutron star (NS) sources requires the
availability of gravitational waveforms with tidal effects accurate up to merger. This article …

Neutron star (NS) equation of state (EoS) insensitive relations or universal relations (UR)
involving neutron star bulk properties play a crucial role in gravitational-wave astronomy …

Gravitomagnetic quasinormal modes of neutron stars are resonantly excited by tidal effects
during a binary inspiral, leading to a potentially measurable effect in the gravitational-wave …

LIGO and Virgo have recently observed a number of gravitational wave (GW) signals that
are fully consistent with being emitted by binary black holes described by general relativity …

GW170817, the milestone gravitational-wave event originated from a binary neutron star
merger, has allowed scientific community to place a constraint on the equation of state of …

We compute the spin-tidal couplings that affect the dynamics of two orbiting bodies at the
leading order in the post-Newtonian (PN) framework and to linear order in the spin. These …

The gravitomagnetic tidal Love number of a slowly rotating body was calculated previously
under the assumption that the velocity perturbation created by the tidal field consists of an …