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Nuclear Fission and Fusion UMA LAD PHY 3305: MODERN PHYSICS DECEMBER 2, 2014.

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Presentation on theme: "Nuclear Fission and Fusion UMA LAD PHY 3305: MODERN PHYSICS DECEMBER 2, 2014."— Presentation transcript:

1 Nuclear Fission and Fusion UMA LAD PHY 3305: MODERN PHYSICS DECEMBER 2, 2014

2 Outline Fission and fusion will be defined. Examples of fission and fusion will be discussed. Modern day applications of these reactions will be discussed. 12/02/2014LAD MODERN PHYSICS2

3 Nuclear Reaction Occurs when a nucleus collides with another particle Example: uranium- 235 decays into barium and krypton 12/02/2014LAD MODERN PHYSICS3 Total Energy released: Q= (m i – m f )c 2

4 Nuclear Fission Nucleus breaks down into many parts Releases kinetic energy Many isotopes decay through induced fission Number of protons and neutrons affects the amount of energy released 12/02/2014LAD MODERN PHYSICS4 Fig. 1. Uranium Fission. “Mousetrap Reactor.” SMU Physics and Astronomy Demonstrations. 2014. Web. 25 Nov. 2014.

5 Chain Reactions Each fission reaction will cause other fission reactions to occur. Critical assembly: ensures that a reaction can sustain itself 12/02/2014LAD MODERN PHYSICS5 The energy released during a chain reaction: E j = E 0 k j

6 Fission Reactor Uranium-235 is used as the fuel Control rods absorb neutrons Neutrons produced from each generation become slower 12/02/2014LAD MODERN PHYSICS6

7 12/02/2014LAD MODERN PHYSICS7 Pressure Water Reactor Fig. 2. A Light-Water Nuclear Fission Reactor for the Production of Electric Power. Digital image. ”Applied Nuclear Chemistry.” UC Davis Chemwiki. UC Davis, n.d. Web. 20 Nov. 2014.

8 Nuclear Fusion Nuclei combine to form heaver nuclei Mass decreases Kinetic energy increases 12/02/2014LAD MODERN PHYSICS8

9 Lawson Criterion For fusion to occur: High temperatures are necessary Reaction must be held: For a certain amount of time A certain density of ions 12/02/2014LAD MODERN PHYSICS9

10 12/02/2014LAD MODERN PHYSICS10 Proton-Proton Cycle End result: helium Energy source of the Sun Fig. 3. Fission in the Sun. “Proton- Proton Chain Reaction.” Wikipedia. Wikimedia Foundation Inc., 2006. Web. 25 Nov. 2014.

11 Fusion in Relation to Stars Carbon Cycle Uses carbon as a catalyst Results in helium Occurs when a star has a high temperature Stellar Collapse- Star collapses into a white dwarf Energy production from fusion no longer matches the gravitational attraction 12/02/2014LAD MODERN PHYSICS11

12 Fusion Reactors Difficult to use as a power source Requires extreme conditions Ways to confine nuclei Magnetic confinement Inertial confinement 12/02/2014LAD MODERN PHYSICS12

13 Conclusion Fission - nucleus breaking down into many parts. Fusion - nuclei combining to form heaver nuclei. Chain reaction - one reaction triggers many other reactions. Fission reactors are used to produce energy. Proton-proton cycle is composed of multiple fusion reactions. 12/02/2014LAD MODERN PHYSICS13

14 Sources Harris, Randy. Modern Physics. 2nd ed. San Francisco: Pearson, 2008. 503-513. Print. Herrmann, Mark. “Plasma Physics: A promising advance in nuclear fusion.” Nature 506 (2014): 302-303. Web. 17 Nov. 2014. Nave, Rod. "Nuclear Fusion." HyperPhysics. Web. 11 Nov. 2014. <http://hyperphysics.phy-astr. gsu.edu/hbase/nucene/fission.html#c1>. Reed, Cameron B. “Neutrons as Party Animals: An Analogy for Understanding Heavy-Element Fissility.” The Physics Teacher 50 (2012): 544-545. Web. 17 Nov. 2014. 12/02/2014LAD MODERN PHYSICS14


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