Speaker
Mr
SK MD Adil Imam
(SINP, Kolkata)
Description
The posterior distributions of nuclear matter properties are reconstructed
using a Bayesian technique from
the EoS of neutron star matter. Appropriate prior distributions are
chosen to put constraints on lower-order
parameters as imposed by the finite nuclei observables. The calculations
are performed on two sets of pseudo
data on the EoS whose real models are known. The accompanying
uncertainties are also greater and the median
values of second or higher order NMPs exhibit considerable deviation
from their true values. The sources of
these inherent uncertainties are discussed.
