activity
20242026
collaborators

7 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

Differentially rotating neutron stars with dark matter cores

Lorenzo Cipriani, Violetta Sagun, Kalin V. Staykov +2

Dark matter is expected to accumulate inside neutron stars, modifying the structure of isolated stars and influencing both the dynamics of binary mergers and the evolution of the r…

nucl-th2025

Color-superconducting quarkyonic matter

Christoph Gärtlein, Oleksii Ivanytskyi, Violetta Sagun +1

We explore the role of color superconductivity in quarkyonic matter under the conditions of color and electric neutrality at - and strong equilibrium, as relevant for neutron st…

astro-ph.HE2025

Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars

Edoardo Giangrandi, Hannes R. Rüter, Nina Kunert +7

Binary neutron star mergers provide insight into strong-field gravity and the properties of ultra-dense nuclear matter. These events offer the potential to search for signatures of…

astro-ph.HE2025

Rapidly spinning dark matter-admixed neutron stars

Lorenzo Cipriani, Edoardo Giangrandi, Violetta Sagun +2

Millisecond pulsars, representing the older neutron star population, are believed to have undergone a prolonged period of dark matter accumulation, resulting in a higher dark matte…