activity
20242026
most citedEffect of symmetry energy on properties of rapidly rotating neutron stars and universal relations

2 citations · 2 across the 3 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2026

ESO Expanding Horizon White Paper: Revealing the properties of matter at supranuclear densities with gravitational waves

Tim Dietrich, Tanja Hinderer, Micaela Oertel +40

Understanding dense matter under extreme conditions is one of the most fundamental puzzles in modern physics. Complex interactions give rise to emergent, collective phenomena. Whil…

astro-ph.HE2025

Thermal conduction and thermopower of inner crusts of magnetized neutron stars

Henrik Danielyan, Arus Harutyunyan, Armen Sedrakian

We compute the thermal conductivity and thermoelectric power (thermopower) of the inner crust of compact stars across a broad temperature-density domain relevant for proto-neutron…

astro-ph.HE2025

Rapidly rotating hot nuclear and hypernuclear compact stars: integral parameters and universal relations

Stefanos Tsiopelas, Armen Sedrakian, Micaela Oertel

In this work, we investigate hot, isentropic compact stars in the limiting cases of static and maximally rotating configurations, focusing on how variations in the symmetry energy…

astro-ph.HE20252 cited

Effect of symmetry energy on properties of rapidly rotating neutron stars and universal relations

Pion Sudarshan Yeasin, Stefanos Tsiopelas, Armen Sedrakian +1

We investigated universal relations for compact stars rotating at the Keplerian (mass-shedding) limit, which is highly relevant for understanding the rapidly rotating objects forme…

astro-ph.HE2025

Topology of the Superconducting Heart of Neutron Stars: Effects of Microphysics and Gravitational-Wave Signatures

Mayusree Das, Armen Sedrakian, Banibrata Mukhopadhyay

We present a general-relativistic study of the distribution of proton superconductivity in strongly magnetized neutron stars (NSs), using the XNS code to solve the coupled Einstein…

gr-qc2025

Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating

Henrique Gieg, Maximiliano Ujevic, Armen Sedrakian +1

We present a new set of numerical-relativity simulations of merging binary neutron stars, aiming to identify possible observable signatures of the slope of the symmetry energy $L_{…