PPT-Working Group on Central Nuclear Reactions/EOS

Pawel Danielewicz NSCLMSU Justin Estee NSCLMSU Chuck Horowitz IU BaoAn Li TAMUC YuGang Ma SINAP Pierre Morfouace NSCLMSU Zhiyu Sun IMP Betty Tsang NSCLMSU Zhigang Xiao . Dubna. , Russia. Avazbek NASIROV. Joint Institute for Nuclear Research. Contents of talk. Short information about synthesis of superheavy elements . . in heavy ion collisions.. 2. Significance of nuclear reactions: . Dubna. , Russia. Avazbek NASIROV. Joint Institute for Nuclear Research. Contents of talk. Short information about synthesis of superheavy elements . . in heavy ion collisions.. 2. Significance of nuclear reactions: . Fission and Fusion. A brief history…. 1919: Ernest Rutherford experimented with bombarding nitrogen gas molecules with alpha particles emitted from bismuth-214. Discovery: faster moving particles were produced, and these could travel farther than the alpha particles!. 北京大学物理学院. . 技术物理系 . • . 裴俊琛. . Junchen. Pei, School of Physics, Peking University . 2016.9, Beijing. Prepared based on many others slides. Introduction. How do we do these experiments?. How . do RIBs . play a role?. Connections to nuclear astrophysics. Sherry Yennello . 2015 EBSS. The nucleus as a liquid drop. N/Z asymmetry. Heat Input. Temperature. Ice (Solid). Atoms consist of a nucleus surrounded by electrons. Chemistry is produced by interactions involving the electrons around the atom. t. his involves small energy changes (~0.01 eV) and can happen at room temperatures. Nuclear chemistry is the study of the structure of and the they undergo.. atomi. c nuclei. changes. Chemical vs. Nuclear Reactions. Elements are Formed in Different Ways in our Universe. Nucleosynthesis. Nucleosynthesis. is the process of element (nuclei) formation.. Three types: . Big Bang nucleosynthesis. . Stellar (star) nucleosynthesis. Unit Test Thursday. Nuclear Radiation. Video. Marie Curie, Nobel Prize Winner . What is Radioactivity?. When nuclei of unstable isotopes gain stability by undergoing changes. These reactions:. are called nuclear reactions. for nuclear structure, reaction mechanisms and nuclear astrophysics. Livius Trache. l-trache@tamu.edu. Cyclotron Institute, Texas A&M University . and. Institute for Physics and Nuclear Engineering Bucharest, Romania. International Partnership for Nuclear Disarmament Verification Looking toward Phase II – Facilitated Discussion Take a “quick look ahead” at some of the questions and issues of the three new Working Groups How do stars work and evolve?. Why do stars shine?. Nuclear reactions. Fusion and fission reactions. How nuclear reactions can create energy. Why is it hard to get fusion nuclear reactions to occur?. …. Nuclear . Astrophysics with exotic nuclei and rare ion beams . Decay spectroscopy for nuclear astrophysics. Livius Trache. Texas A&M University . and. IFIN-HH Bucharest. Exotic Beam Summer School 2012 . Accomplishments and Upcoming . Workshop . . Catherine Romano. Cross Section Evaluation Working Group Meeting. (CSEWG). November 6-9, 2017. Brookhaven, NY. Recent Events in Nuclear Data.