Présidents de session
Theoretical (microscopic) calculations of neutron rich dense nuclear matter
- Pawel Danielewicz (Michigan State University)
Theoretical (microscopic) calculations of neutron rich dense nuclear matter
- Rémi Bougault (LPC Caen)
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Christian Drischler (Ohio University)09/09/2024 14:00Microscopic calculations of neutron-rich dense nuclear matterInvited Presentation
In recent years, significant advances have been made in constraining the dense matter equation of state (EOS) from, e.g., multi-messenger astronomy, chiral effective field theory (EFT), novel experimental campaigns such as PREX-II and CREX, and heavy-ion collisions. However, many key questions remain, especially regarding the composition and EOS of the dense matter in the inner cores of heavy...
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Jing Ye (Southeast University)09/09/2024 14:30Oral Presentation
The meaningful correlations between the zero-sound modes and the stiffness of the nuclear equation of state (EOS) are uncovered in symmetric nuclear matter with the relativistic mean-field (RMF) theory. We found that the high-density zero-sound modes merely exist in models with the stiff EOS. While the soft RMF EOS are usually characteristic of the inclusion of the $\omega$-meson...
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Panagiota Papakonstantinou (IBS/IRIS)11/09/2024 09:45Microscopic calculations of neutron-rich dense nuclear matterOral Presentation
The properties of neutron-rich nuclear systems are largely determined by the density dependence of the nuclear symmetry energy. Experiments aiming to measure the neutron skin thickness [1,2] and astronomical observations of neutron stars and gravitational waves [3,4] offer valuable information on the symmetry energy at sub- and supra-saturation densities, respectively.
The KIDS theoretical...
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