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Slide 1Systematics of fusion probability in reactions leading to super-heavy nuclei Ning Wang ( ) Guangxi Normal University www.imqmd.com 2011 Dec., Beijing Slide 2 N. Wang…

Slide 1 It is my great pleasure to say some words on this occasion to celebrate Prof. Joe. Natowitz’s achievement on this workshop. Because unexpected delay for my visa…

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…

Ning Wang1, Min Liu1, Xi-Zhen Wu2, Jie Meng3 Isospin effects in nuclear mass models Nuclear Structure and Related Topics (NSRT15), 2015.7.14-18, DUBNA 1 Guangxi Normal University,…

The High-Density Symmetry Energy in Heavy Ion Collisions Int. School on Nuclear Physics: Probing the Extremes of Matter with Heavy Ions, Erice, Sept. 16-24 2012 Hermann Wolter…

Hyperon Star Model Ilona Bednarek Ustroń, 2009 Typical neutron star parameters: Neutron stars are the most compact objects M ~ 1.4 MS 1.44 MS the largest precisely known…

It is my great pleasure to say some words on this occasion to celebrate Prof. Joe. Natowitz’s achievement on this workshop. Because unexpected delay for my visa process,…

The High-Density Symmetry Energy in Heavy Ion Collisions Int. School on Nuclear Physics: Probing the Extremes of Matter with Heavy Ions, Erice, Sept. 16-24 2012 Hermann Wolter…

Measurement of the neutron skin of heavy nuclei Measurement of the neutron skin of heavy nuclei G. M. Urciuoli INFN Sezione di Roma Why do we measure the neutron skin of…