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The LSND-ino (with help from Extra Dimensions)

The LSND-ino (with help from Extra Dimensions). Tom Weiler Vanderbilt University. LSND data and inference. Third d m 2 , and so fourth neutrino mass-state n 4. Z-width requires n 4 to be gauge-singlet – “sterile’. Incredible, yes; Credible, ????.

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The LSND-ino (with help from Extra Dimensions)

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  1. The LSND-ino(with help from Extra Dimensions) Tom Weiler Vanderbilt University IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  2. LSND data and inference Third dm2, and so fourth neutrino mass-state n4 Z-width requiresn4 to be gauge-singlet – “sterile’ IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  3. Incredible, yes; Credible, ???? • Fails S. Biller’s “redundancy criterion (and his second redundancy criterion too) • Would I bet money on it being right? (I’d love to bet some of Don Perkin’s money on it, and WIN) • Mini-BooNE coming very soon, to a conference near you. IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  4. Failure of LSND stable sterile in 4D IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  5. Proposed models (some dead) • Three (or Four) Nu with broken CPT DEAD (ALIVE) • Lepton-number violating muon decay DEAD • Five Nu oscillations • Low reheat-temperature cosmology • QGravity decoherence with broken CPT • MaVans (mass-varying neutrinos) • Four Nu with decay • Extra-dimensional geodesics for sterile neutrinos IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  6. Commonality of models • Have new parameters/new physics 5th neutrino, DK to scalar, more spacetime, quantum gravity, new cosmology, coupling to DarkEnergy, ….. o Way beyond Standard Model o Testable predictions IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  7. KeV-MeV n4 model IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  8. Fits Note the parameter equivalences IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  9. Brane-Bulk resonance model IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  10. In QG/StringTheory, brane is dynamical, fluctuating due to Quantum MechanicsThermal MechanicsIn-Brane stresses (e.g. EM vs. gravity)Out of Brane experiences (e.g. trans-brane gravity) IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  11. A tale of two geodesics IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  12. BB-resonance which is the (fluctuation aspect ratio)2 IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  13. Two-flavor resonances Define |na>U = |n4> - < ns | n4 > | ns > IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  14. Brane-Bulk Resonant Oscillation CDHS In nu and nubar channels (gravity doesn’t care) IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  15. Goodbye CDHS! CDHS IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  16. Examples: n00 MeV resonance And significant nm disappearance for stopped-pion source (SNS) IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  17. Example: 40 MeV resonance IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

  18. Conclusions If LSND is correct, then …. theory needs a HUGE accommodation. (In)validation is “just around the corner, With Fermilab’s MiniBooNE experiment (altho some LSND models predict null MiniBooNE, positive something else) IOP/CfCP Neutrino Meeting, June 29, 2005, Tom Weiler, Vanderbilt University

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