Speaker
Arunava Mukherjee
(Saha Institute of Nuclear Physics, Kolkata)
Description
Neutron star equations of state based on Skyrme-interaction are one of the most widely used models to describe ultra-dense nuclear matter at the interior of these degenerate stars. In this presentation, I will discuss the effect of various Skyrme parameters on the stellar structural properties of a neutron star and its observables. I will also briefly present the potential source of biases in Bayesian inferences from astrophysical observations of gravitational waves and x-ray emissions, along with some of the possible avenues to mitigate them.
Author
Arunava Mukherjee
(Saha Institute of Nuclear Physics, Kolkata)
