PPT-Nuclear Energy in the 21

st Century Liping Gan   University of North Carolina Wilmington   Outline Introduction What is nuclear energy Early history of nuclear power Current status Critical Issues Future of nuclear energy. Milos. June 2011. . V. . Kaplunovsky. . A. . Dymarsky. , D. . Melnikov. and S. Seki, . Introduction. In recent years . holography. or . gauge/gravity duality. has provided a new tool to handle strong coupling problems.. power.  . S.Tyutyunnikov. Joint Institute for Nuclear Research, . Dubna. , Russia. Based on the use of relativistic nuclear technology (RNT) a new scheme electronuclear method aims at forming in the volume of the active zone (AZ) are significantly more stringent than the fission of the neutron spectrum and use this spectrum for production of energy and recycling of spent nuclear fuel (SNF), as well as for transmutation of long-lived components of radioactive waste (RAW) of nuclear power.. Paula L. . Diaconescu. Why talk about nuclear energy?. http://copper.chem.ucla.edu/pldgroup/index.htm. Whitesides. . Science. 2007. The news. Nuclear power now generates 15% of the world's electricity.. By: Aiden Cook, Kaitlyn Hemauer,. Abbey Loar, and . Elizabeth Rogers. How Does It Work?-Abbey. Nuclear Power Plants and fossil fuels are almost the same.. To keep the water under pressure you use a Pressurized Water Reactor. . Is radiation dangerous? . Is nuclear power a good choice?. . What is nuclear energy?. Are nuclear energy and nuclear bombs both dangerous? . Guiding Questions. The Power of the Nucleus. Bravo – 15,000 kilotons. Atomic . and Nuclear Physics. Dr. David . Roelant. Atomic and Molecular Weight. Problem 1. Using the data in the table below, compute the atomic weigh of naturally occurring oxygen.. Isotope. Abundance. Nuclear physics . . what’s inside the nucleus and what . holds it together . . what is radioactivity, half-life . . carbon dating . . Nuclear energy. nuclear fission. nuclear fusion. Presentation by Peter Huessy of the Mitchell Institute/AFA to the SDC Symposium, June 20-21, 2016 Albuquerque, New Mexico. WHERE HAVE WE BEEN? . WHAT ARE WE TRYING TO DO? . WHERE ARE WE TRYING TO GO?. Shuting Fan. Co-TERMINAL, MECHANICAL ENGINEERING. Motivation. -Why I choose nuclear fusion as my topic today?. Intern, EAST Tokamak Design Division, Institute of Plasma Physics, China. Interested in learning the physics behind it and its potential economical and environmental value . GGI May 2011. . V. . Kaplunovsky. . A. . Dymarsky. , D. . Melnikov. and S. Seki, . Introduction. In recent years . holography. or . gauge/gravity duality. has provided a new tool to handle strong coupling problems.. Tanju Sofu. Argonne National Laboratory. Fermilab. Colloquium. June 28, 2017. Fermi National Accelerator Laboratory. Chicago Pile 1. Beginning of the road. …. Argonne’s EBR-I . p. roduces . f. irst ever nuclear . Learning Goal . Write a balanced nuclear equation showing mass numbers and atomic numbers for radioactive decay.. Balancing Nuclear Equations. In a process called . radioactive decay. , the nucleus breaks down by emitting radiation. . WJEC Physics Unit 2 - 2.9. Nuclear Fusion. H – Deuterium nucleus. 2. 1. H – Deuterium nucleus. 2. 1. Two deuterium nuclei approach one another. The two nuclei collide. Nuclear Fusion. H –nucleus. A naturally . radioactive element . will . emit . energy without the absorption of energy from an outside source. . The nucleus of an element becomes radioactive because of an unstable ratio of protons to neutrons in the nucleus..