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experiment X

experiment X. n ’ s per day : > 100 per day total statistics : > 10 6 over 10yr energy : 0.1 ~ 10,000 TeV. IceCube… 1 million neutrinos. analytic IceCube simulation TeV neutrinos oscillate, propagate, regenerate and decay… coherently

orlando-conley
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experiment X

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  1. experiment X • n’sper day : > 100 per day • total statistics : > 106over10yr • energy : 0.1 ~ 10,000 TeV

  2. IceCube… 1 million neutrinos analytic IceCube simulation TeV neutrinos oscillate, propagate, regenerate and decay… coherently new physics signatures unmatched sensitivity Gonzalez-Garcia, Maltoni

  3. your own IceCube simulation • # events = ∫ Area Timefn{lm/ln } • Input: A (Em) from astro-ph/0305196  Cuts: • length of muon track > 300 m • number of channels as a function of zenith angle q •  implemented as integration limits on the muon • range and energy as a function of zenith

  4. Neutrinos • oscillate • interact • regenerate • tau decay

  5. new physics with atmospheric neutrinos

  6. New Physics with the Atmospheric Beam with induced by new vector/tensor-like interactions

  7. New Physics with the Atmospheric Beam: Examples • Violation of the equivalence principle: • Violation of Lorentz invariance:

  8. new physics with atmospheric neutrinos

  9. Total 455,246 (10 years)

  10. Cosmic neutrino beam from the decay of pions e :  :  ~ 1 : 2 : <10-5@ the source e :  :  ~ 1 : 1 : 1 @ the detector (maximal   mixing) • Or, • zero mass eigenstates in vacuum • neutrino decay • neutrinos of varying mass • …..

  11. TeV B L A Z A R 1ES 1959+650 a posteriori coincidence TeV Flux (Crab) H. Krawczynski et al, 2004ApJ,601 151K ‘Multiwavelength Observations of Strong Flares from the TeV Blazar 1ES 1959+650’ 10 keV Flux (keV-1 cm-2 s-1) “orphan” flare PRELIMINARY

  12. Neutrino Beams: Heaven & Earth NEUTRINO BEAMS: HEAVEN & EARTH Black Hole Radiation Enveloping Black Hole p + g -> n + p+ ~ cosmic ray + neutrino -> p + p0 ~ cosmic ray + gamma

  13. Neutrino Beams: Heaven & Earth g ~ n

  14. g-rays fromp0decay discovered ? 1 <  < 8 accelerator beam dump (hidden source) transparent source p0 = p+ = p- ∫ En Nn (En) = ∫EgNg (Eg) n flux predictedobserved g-ray flux ~20 per km2 RX J1713-3946 per year (galactic center)

  15. HESS: RX J1713 Spectrum 18 h 2003 data Resolution ~10 arcmin First resolved TeV image

  16. energy conservation and cascading E-2.8 E-2 TeV G m p0

  17. Input: transparent source of 1 Crab with 2 < Eg < 20 TeV gamma ray slope 2.8 2.5 2.2 1E 1959+680

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