In this work, we consider polar perturbations, and we calculate the frequency and dam**
time of the quadrupolar fundamental f-mode of compact objects, constructed using a wide …

The nature of the highly dense matter inside the supernova remnant compact star is not
constrained by terrestrial experiments and hence modeled phenomenologically to …

We present fully general relativistic 3D numerical simulations of accretion-induced collapse
(AIC) of white dwarfs (WDs). We evolve three different WD models (non-rotating, rotating at …

Three-dimensional modeling has reached a level of maturity to provide detailed predictions
of the gravitational wave emission in neutrino-driven core collapse supernovae. We review …

Certain relations among neutron-star observables that are insensitive to the underlying
nuclear matter equation of state are known to exist. Such universal relations have been …

We present an analysis of gravitational wave (GW) predictions from five two-dimensional
core collapse supernova (CCSN) simulations that varied only in the equation of state (EOS) …

Quasinormal modes of neutron stars are an exciting prospect for analyzing the internal
composition of neutron stars and studying matter at high densities. In this work, we focus on …

Aims. In this work we extended an energy-integrated neutrino transport method to facilitate
efficient, yet precise, modeling of compact astrophysical objects. We particularly focus on …

Gravitational wave signals from core-collapse supernovae are one of the important
observables for extracting the information of dense matter. To extract the properties of …

Recent studies have revealed that certain nuclear parameters are more dominant than
others in governing global neutron star properties, such as its structure or oscillation mode …