Speaker
Prof.
William Lynch
Description
The Equation of State (EoS) of Asymmetric matter governs the properties of dense matter within neutron stars and influences the properties of the neutrino-sphere and the proto-neutron star created during a core-collapse supernova. Constraining the EoS via laboratory experiments constitutes one the principal objectives of nuclear science. During this presentation, I will review the status of current constraints and discuss current efforts to improve the constraints both at sub-saturation and supra-saturation densities.
| List of tracks | Femtoscopy in A+A, p+p , p+A and e+-e- collisions at relativistic, intermediate and low energies |
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Primary author
Prof.
William Lynch
