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SCL for 1-MW AGS Upgrade

SCL for 1-MW AGS Upgrade. Alessandro G. Ruggiero Brookhaven National Laboratory. NuFact 03 Workshop Columbia University, New York June 5-11, 2003. Goal & Comparison. Upgrade with the AGS Booster ?. Upgrade with Super–Conducting Linac. Why a Super-Conducting Linac.

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SCL for 1-MW AGS Upgrade

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  1. SCL for 1-MW AGS Upgrade Alessandro G. Ruggiero Brookhaven National Laboratory NuFact 03 Workshop Columbia University, New York June 5-11, 2003

  2. Goal & Comparison NuFact'03 Workshop Columbia University, New York

  3. Upgrade with the AGS Booster ? NuFact'03 Workshop Columbia University, New York

  4. Upgrade with Super–Conducting Linac NuFact'03 Workshop Columbia University, New York

  5. Why a Super-Conducting Linac NuFact'03 Workshop Columbia University, New York

  6. The 1.2-GeV SCL for the 1-MW AGS Upgrade NuFact'03 Workshop Columbia University, New York

  7. SCL Layout NuFact'03 Workshop Columbia University, New York

  8. Front-End NuFact'03 Workshop Columbia University, New York

  9. SCL Site and Layout NuFact'03 Workshop Columbia University, New York

  10. Injector and AGS Parameters for 1-MW Upgrade NuFact'03 Workshop Columbia University, New York

  11. SCL Components NuFact'03 Workshop Columbia University, New York

  12. A Cryo-Module NuFact'03 Workshop Columbia University, New York

  13. Warm Insertions (why warm?) NuFact'03 Workshop Columbia University, New York

  14. General Parameters of SCL Sections NuFact'03 Workshop Columbia University, New York

  15. Other SCL Parameters NuFact'03 Workshop Columbia University, New York

  16. Project Cost NuFact'03 Workshop Columbia University, New York

  17. Super Neutrino Beam Geographical Layout NuFact'03 Workshop Columbia University, New York

  18. 3-D Neutrino Super Beam Perspective NuFact'03 Workshop Columbia University, New York

  19. Advantages of a Very Long Baseline  neutrino oscillations result from the factor sin2(Dm322L / 4E) modulating the n flux for each flavor (here nm disappearance)  the oscillation period is directly proportional to distance and inversely proportional to energy  with a very long baseline actual oscillations are seen in the data as a function of energy  the multiple-node structure of the very long baseline allows the Dm322 to be precisely measured by a wavelength rather than an amplitude (reducing systematic errors) NuFact'03 Workshop Columbia University, New York

  20. BNL Homestake 2540 km BNL  Homestake Super Neutrino Beam NuFact'03 Workshop Columbia University, New York

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