Dr. Deepak Kumar

**Affiliation:** IISER-Bhopal, India

**Title:** Correlations of nuclear matter EOS with the non-radial f mode oscillations of neutron stars

**Abstract:** Constraining the equation of state of a neutron star is a big question. We will discuss that the measurements of mode oscillations can constraint the different parts of the equation of state. We investigate the intricate relationships between the non-radial f mode oscillation frequencies of neutron stars (NS)s and the corresponding nuclear matter equation of state (EOS) using a machine learning (ML) approach within the ambit of the relativistic mean field (RMF) framework for nuclear matter. With two distinct parameterizations of the Walecka model, namely, (1) with non-linear self interactions of the scalar field (NL) and, (2) a density dependent Bayesian model (DDB), we perform a thorough examination of the f mode frequency in relation to various nuclear saturation properties. The correlations between the f mode frequencies and nuclear saturation properties reveal, through various analytical and ML methods, the complex nature of NSs and their potential as the cosmic laboratory for studying extreme states of matter.

Design: TEMPLATED Images: G. Andre Oliva.