activity
20242026
most citedCrust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2

6 citations · 8 across the 5 of their papers we have counts for

collaborators

8 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

Probing neutron star interiors and the properties of cold ultra-dense matter with the SKAO

Avishek Basu, Vanessa Graber, Marcus E. Lower +19

Matter inside neutron stars is compressed to densities several times greater than nuclear saturation density, while maintaining low temperatures and large asymmetries between neutr…

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…

nucl-th20251 cited

Properties of Neutron Stars with Hyperons within a Relativistic Metamodel

Prasanta Char, Chiranjib Mondal, Timothé Alezraa +2

In this work, we study the effects of -hyperons on neutron star properties employing a metamodel framework for the equation of state (EoS). Different choices for defining the hy…

astro-ph.HE2025

Stellar properties indicating the presence of hyperons in neutron stars

Andreas Bauswein, Aristeidis Nikolaidis, Georgios Lioutas +7

We describe distinctive stellar features indicating the presence of hyperons in neutron stars as compared to purely nucleonic systems. A strongly negative curvature of the mass-rad…

astro-ph.HE20256 cited

Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2

P. J. Davis, H. Dinh Thi, A. F. Fantina +3

The equation of state (EoS) is a needed input to determine the neutron-star global properties and to relate them. It is thus important to provide consistent and unified EoSs to avo…