Nuclear structure and reactions @IN2P3 Selected Higlights Shell evolution and nuclear interactions Reactions with weakly bound nuclei Nuclear Astrophysics.
Lesson 15 The Transuranium Elements. The Basics 118 known elements, 1-118 All elements beyond 92 man-made.
Isospin dependence and effective forces of the Relativistic Mean Field Model Georgios A. Lalazissis Aristotle University of Thessaloniki, Greece Georgios.
*) for a period of 2008-13 Polish nuclear structure theory (NST) in numbers*) Brief overview of scientific activities Physics highlights - personal selection.
E. De Filippo (INFN Catania) for the REVERSE / ISOSPIN collaboration Time sequence and isoscaling in neck fragmentation Fragments production in peripheral.
F. Sammarruca, University of Idaho [email protected] Supported in part by the US Department of Energy. From Neutron Skins to Neutron Stars to Nuclear.
Probe the structure & spectroscopy at large isospin Measure unbound states detection devices
ISOSPIN-MIXED X HYPERNUCLEAR STATES AND (K,K) REACTIONS
Direct reactions to unbound states ESNT 4-6Fev. 08 CEA-SPhN [email protected] SPIRALSPIRAL2EURISOL Neutron-skin structure and shell evolution of weakly-bound.
12/17/20151NuPECC Meeting - BentleyOverview Gamma-ray Spectroscopic Studies of Exotic Nuclei: Towards NuSTAR Mike Bentley (University of York, UK) Gamma-ray.
E. De Filippo (INFN Catania) for the REVERSE / ISOSPIN collaboration
F. Sammarruca, University of Idaho fsammarr@uidaho
