Slide 1 Neutron Number N Proton Number Z a sym =30-42 MeV for infinite NM Inclusion of surface terms in symmetry Slide 2 The National Superconducting Cyclotron Laboratory…

Slide 1 Determination of Density Dependence of Nuclear Matter Symmetry Energy in HIC’s ISOSPIN PHYSICS AND LIQUID GAS PHASE TRANSITION, CCAST, Beijing, Aug. 19-21, 2005…

PowerPoint Presentation Objectives and benefits to the US nuclear physics programs Accomplishments so far Opportunities and Challenges Nuclear Theory Program Division of…

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Constraining the EoS and Symmetry Energy from HI collisions Statement of the problem Demonstration: symmetric matter EOS Laboratory constraints on the symmetry energy from…

Diapositiva 1 E. De Filippo (INFN Catania) for the EXOCHIM collaboration Correlations between isospin dynamics and IMF emission time-scales: a probe for the symmetry energy…

幻灯片 1 Constraints on symmetry energy and n/p effective mass splitting with HICs Yingxun Zhang (张英逊) China Institute of Atomic Energy HIRFL-RIBLL合作体第2次会议，上海…

幻灯片 1 Constraints on symmetry energy and the n/p effective mass splitting Symmetry energy: Besides depending on the nuclear density, the symmetry energy also depends…

Constraining the EoS and Symmetry Energy from HI collisions Statement of the problem Demonstration: symmetric matter EOS Laboratory constraints on the symmetry energy from…