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

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

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

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

Nuclear Fission and FusionUMA LAD

PHY 3305: MODERN PHYSICS

DECEMBER 2, 2014

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

Outline • Fission and fusion will be defined.

• Examples of fission and fusion will be discussed.

• Modern day applications of these reactions will be discussed.

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Nuclear Reaction• Occurs when a nucleus collides with another particle

• Example: uranium- 235 decays into barium and krypton

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Total Energy released:Q= (mi – mf)c2

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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

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Fig. 1. Uranium Fission. “Mousetrap Reactor.” SMU Physics and Astronomy Demonstrations. 2014. Web. 25 Nov. 2014.

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Chain Reactions• Each fission reaction will cause other fission reactions to occur.

• Critical assembly: ensures that a reaction can sustain itself

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The energy released during a chain reaction:Ej = E0kj

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Fission Reactor• Uranium-235 is used as the fuel• Control rods absorb neutrons

• Neutrons produced from each generation become slower

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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. 

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Nuclear Fusion• Nuclei combine to form heaver nuclei

• Mass decreases

• Kinetic energy increases

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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

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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.

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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

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Fusion Reactors• Difficult to use as a power source

• Requires extreme conditions

• Ways to confine nuclei• Magnetic confinement

• Inertial confinement

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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.

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SourcesHarris, 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.

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