Hall A Collaboration Meeting, December 13-14, 2007 E03-104: Probing the Limits of the Standard Model of Nuclear Physics with the 4 He(e,ep) 3 H Reaction.
7-1 Fission Readings: Modern Nuclear Chemistry, Chapter 11; Nuclear and Radiochemistry, Chapter 3 General Overview of Fission Energetics The Probability.
Pavel Stránský 29 th August 2011 W HAT DRIVES NUCLEI TO BE PROLATE? Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México Alejandro.
10-1 Fission General Overview of Fission The Probability of Fission §The Liquid Drop Model §Shell Corrections §Spontaneous Fission §Spontaneously Fissioning.
7-1 RFSS: Lecture 7 Fission Readings: Modern Nuclear Chemistry, Chapter 11; Nuclear and Radiochemistry, Chapter 3 General Overview of Fission Energetics.
NSTAR2007@Bonn 9/8/07-1 Simon Capstick, Florida State University.
Some questions on quantum anomalies Roman Pasechnik Moscow State University, Moscow & Bogoliubov Lab of Theoretical Physics, JINR, Dubna 46-th Cracow School.
1 Alpha Decay Energetics of Alpha Decay Theory of Alpha Decay Hindrance Factors Heavy Particle Radioactivity Proton Radioactivity Identified at positively.
Role of mass asymmetry in fusion of super-heavy nuclei K. Siwek- Wilczyńska, I. Skwira-Chalot, J. Wilczyński aim to compare our model predictions with.
Dinuclear system model in nuclear structure and reactions.
Role of mass asymmetry in fusion of super-heavy nuclei
A.What is the EOS? 0. Relationship to energy and to nuclear masses 1. Important questions B. What observables are sensitive to the EOS and.