activity
20222026
most citedImpact of the equation of state on - and - mode oscillations of neutron stars

56 citations · 56 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

Newtonian I-Love-Q relations: An enthalpy-based approach

Athul Kunjipurayil, J. Piekarewicz

We present a pedagogical introduction to the I-Love-Q relations within Newtonian gravity using an enthalpy-based formulation of stellar structure. Introducing the specific enthalpy…

nucl-th2026

Thermodynamic versus Dynamical Description of the Neutron-Star Crust-Core Instability: Implications for Crustal Observables

Athul Kunjipurayil, J. Piekarewicz

We investigate the crust-core transition in neutron stars using both thermodynamic and dynamical descriptions of the instability. In the thermodynamic approach, the transition is i…

nucl-th2025

Elucidating the role of the surface energy in density functional theory

Md Jafrul Islam, Athul Kunjipurayil, J. Piekarewicz +1

The saturation of symmetric nuclear matter -- reflected in the nearly constant interior density of heavy nuclei -- is a defining property of nuclear matter. Modern relativistic ene…

nucl-th2025

Role of the isovector spin-orbit potential in mitigating the CREX-PREX dilemma

Athul Kunjipurayil, Marc Salinas, J. Piekarewicz

Pioneering electroweak measurements of the neutron skin thickness in lead-208 and calcium-48 are challenging our understanding of nuclear dynamics. Many theoretical models suggest…

nucl-th2022★ 56 cited

Impact of the equation of state on - and - mode oscillations of neutron stars

Athul Kunjipurayil, Tianqi Zhao, Bharat Kumar +2

We investigate the impact of the neutron-star matter equation of state on the - and -mode oscillations of neutron stars obtained within the Cowling approximation and linear…

nucl-th2022

Radial oscillations in neutron stars from unified hadronic and quarkyonic equation of states

Souhardya Sen, Shubham Kumar, Athul Kunjipurayi +3

We study radial oscillations in non-rotating neutron stars by considering the unified equation of states (EoSs), which support the 2 M star criterion. We solve the Sturm-Li…