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High Energy Propulsion

High Energy Propulsion. Brice Cassenti University of Connecticut. High Energy Propulsion. Fusion Annihilation Photon. Fusion Energy. Binding energy Reactions Propulsion. Binding Energy. Some Fusion Reactions. Nuclear Reactions. DT Fusion Reaction Uranium Fission Lithium Fission.

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High Energy Propulsion

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  1. High Energy Propulsion Brice Cassenti University of Connecticut

  2. High Energy Propulsion • Fusion • Annihilation • Photon

  3. Fusion Energy • Binding energy • Reactions • Propulsion

  4. Binding Energy

  5. Some Fusion Reactions

  6. Nuclear Reactions • DT Fusion Reaction • Uranium Fission • Lithium Fission

  7. Fusion Reactions • The DT reaction • And Lithium fission reaction • Are equivalent to

  8. Reaction Cross-Section

  9. Reaction Kinetics • Rate - • Parameter - • Velocity depends on temperature • k is Boltzmann’s constant

  10. Rate vs. Temperature http://www.google.com “nuclear fusion reactor pictures”

  11. Thermonuclear Weapon

  12. Magnetic Confinement Fusion PowerTokamak http://upload.wikimedia.org/wikipedia/commons/4/4b/Tokamak_fields_lg.png

  13. Magnetic Confinement Fusion PowerMirror http://www.google.com “magnetic mirror nuclear fusion reactor pictures”

  14. Inertial Confinement Fusion Power

  15. Fusion Rockets • Magnetic Mirror • End fields unequal: preferential exhaust • Tokamak • Power to expel high speed plasma • Inertial Confinement • Magnetic nozzles align pellet products

  16. Orion

  17. Daedalus StudyBritish Interplanetary Society From Nicolson “The Road to the Stars”

  18. Daedalus http://www.grc.nasa.gov/WWW/PAO/images/warp/warp44.gif

  19. Medusa http://en.wikipedia.org/wiki/File:MedusaNuclearPropulsionOperatingSequenceDrawing.png

  20. Medusa Specific Impulse: 100,000-500,000 http://en.wikipedia.org/wiki/File:MedusaNuclearPropulsionOperatingSequenceDrawing.png

  21. Matter-Antimatter Annihilation • Positron-Electron Annihilation

  22. Antiproton-Uranium Nucleus Annihilation + p p n

  23. Courtesy of G. Smith

  24. Pellet Ignition

  25. Tritium Fuel Considerations • Tritium is naturally radioactive • Beta decay • Half-life ~12 years • Tritium requires cryogenic storage • Lithium-6 is not radioactive • Lithium-6 does not require cryogenic storage

  26. Pellet Construction

  27. Hybrid Fusion-Fission Nuclear Pulse Propulsion • Use of Li6 • Reduces tritium handling problems • Decreases specific impulse • System can be developed in a two step process • Use fusion to boost the specific impulse of a pulse fission rocket • Evolve to a full hybrid system

  28. Typical PelletGeometry • Core radius 0.05 mm • Fuel Radius 1.00 cm • Tungsten Shell Thickness 0.10 mm • Antiproton Beam Radius 0.10 mm • Uranium Hemisphere Radius 0.30 mm

  29. Typical Pellet Performance • Antiproton Pulse 2x1013 for 30 ns • Maximum Field 24 MG • Pellet Mass 3.5 g • Specific Impulse • 600,000 s for 100% fusion • 200,000 s for 10% fusion • 3,000 s for contained fusion

  30. Exotic Propulsion Alternatives

  31. Sanger Electron-PositronAnnihilation Rocket By G. Matloff

  32. Proton-Antiproton Reaction

  33. Proton-Antiproton Reaction

  34. Proton-Antiproton Reaction

  35. Proton-Antiproton Reaction

  36. Proton-Antiproton Reaction +

  37. Proton-Antiproton Reaction +

  38. Pion Rocket Isp: 10,000,000 sec By R. Forward

  39. References • Kammash, T., (editor), Fusion Energy in Space Propulsion, Volume 167 Progress in Astronautice and Aeronautics, American Institute of Aeronautics and Astronautics, Washington, DC,, 1995. • Kammash, T, Fusion Reactor Physics, Ann Arbor Physics, Inc. Ann Arbor, MI, 1976. • Manheimer, W.M., An Introduction to Trapped-Particle Instability in Tokamaks, Energy Research and Development Administration, Washington, DC, 1972. • Miley, G.K., Fusion Energy Conversion, American Nuclear Society and U.S. Energy research and Development Administration, Chicago, 1976. • Miyamoto, K., Plasma Physics for Nuclear Fusion, The MIT Press, Cambridge, MA, 1987. • Vedenov, A.A., Theory of Turbulent Plasma, National Aeronautics and Space Administration, National Science Foundation, and Isreal Program for Scientific Translations, Jerusalem, 1966.

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