Neutron Star Properties and Femtoscopic Constraints

by Valentina Mantovani Sarti (TUM), Valentina Mantovani Sarti (TUM)

Wednesday 2 Jul 2025, 11:00 → 12:00 Europe/Berlin

5101.EG.024 (Seminar Room)

Zoom Room:

https://cern.zoom.us/j/62412236769?pwd=Dl6UCAc4008Wtx9LDBTSSOrj99FJlA.1
Meeting ID: 624 1223 6769
Passcode: 294336

Abstract:

We construct the equation of state of hypernuclear matter and study the structure of neutron stars employing a chiral hyperon-nucleon interaction of the Jülich-Bonn group tuned to femtoscopic $\Lambda p$ data of the ALICE collaboration, and $\Lambda\Lambda$ and $\Xi$N interactions determined from Lattice QCD calculations by the HAL QCD collaboration that reproduce the femtoscopic $\Lambda\Lambda$ and $\Xi^-p$ data. We employ the ab-initio microscopic Brueckner--Hartree--Fock theory extended to the strange baryon sector. A special focus is put on the uncertainties of the hyperon interactions and how they are effectively propagate to the composition, equation of state, and mass-radius relation of neutron stars. To such end, we consider the uncertainty due to the experimental error of the femtoscopic $\Lambda p$ data used to fix the chiral hyperon-nucleon interaction and the theoretical uncertainty, estimated from the residual cut-off dependence of this interaction.

Slides