Présidents de session
Overview
- Anthea FANTINA ({CNRS}UPR3266)
The status of current constraints on the symmetry energy and generally nuclear equation of state (EoS) from laboratory measurements and astrophysical observations is discussed. Determination of the symmetry energy from data requires knowledge of the EoS of symmetric matter, and the heavy-ion collisions (HIC) are the only means of constraining EoS experimentally at supranormal densities. ...
I present the experimental observables which have been identified by present transport approaches as being sensitive to
the potential among nucleons and explicitly to the nuclear equation of state. This is followed by a discussion
which conclusions can be drawn presently and which variables are presently considered as most promising to come to firm conclusions about the different parts of...
