1 / 45

Revolution within ICECUBE Horizons

Revolution within ICECUBE Horizons. Icecube 2013. AUGER. GZK. Gamma-Neutrino-UHECR in sky. The Map CONNECTION: Up dated ARGO Ricap Di Sciascio and ICECUBE Desiati 2013. PLANCK AND AUGER with TA ..from 55 EeV. Last TA and AUGER and Multiplet events at 20 EeV.

kacy
Download Presentation

Revolution within ICECUBE Horizons

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Revolution within ICECUBE Horizons DF in ERICE 23 September: Neutrino Revolution

  2. Icecube 2013 AUGER GZK Gamma-Neutrino-UHECR in sky DF in ERICE 23 September: Neutrino Revolution

  3. The Map CONNECTION: Up dated ARGO Ricap Di Sciascio and ICECUBE Desiati 2013 DF in ERICE 23 September: Neutrino Revolution

  4. PLANCK AND AUGER with TA ..from 55 EeV DF in ERICE 23 September: Neutrino Revolution

  5. Last TA and AUGER and Multiplet events at 20 EeV DF in ERICE 23 September: Neutrino Revolution

  6. Fermi gamma sources and UHECR DF in ERICE 23 September: Neutrino Revolution

  7. Neutrino May day 13 Madison USA2+ 26 events If 10-12 of the 28 eventsare atmospheric than the 7 muon tracks must be mostly of those family.. But why the remaining 18 or 16 events are muon free..? DF in ERICE 23 September: Neutrino Revolution

  8. Horizontal or inclined eventsCascades and tracks DF in ERICE 23 September: Neutrino Revolution

  9. DF in ERICE 23 September: Neutrino Revolution

  10. Showering versus tracks: tau are sphere cascades below PeV DF in ERICE 23 September: Neutrino Revolution

  11. Somehow the 28 are puzzling • No GZK..otherwise peak at EeV no PeV • No Fermi power -2: more PeVs events otherwise..NEED of a CUTOFF • No Prompt neutrinos: too many and too few muon neutrinos: expected 1:1..we have 1:4 • No Extragalactic or Galactic points..but smeared areas ..maybe like TeVs ones Puzzling muon paucity or absence DF in ERICE 23 September: Neutrino Revolution

  12. Where we are looking in the flux map of the universe DF in ERICE 23 September: Neutrino Revolution

  13. DF in ERICE 23 September: Neutrino Revolution

  14. The Flavor Sorpasso revolution • The high energy atmospheric neutrinos are ruled by muon ones leading to tracks • CC Electrons, CC Tau and NC neutrino may lead to spherical shower events: Cascade Shower, a ball of lights • The 28 events are 21 Cascade (Shower) • While only 7 muon tracks: so most atmospheric ones..making muon poor the extraterrestrial ones DF in ERICE 23 September: Neutrino Revolution

  15. DF in ERICE 23 September: Neutrino Revolution

  16. Expected flux a year ago 2012: just EeV GZK neutrino, no PeV ones DF in ERICE 23 September: Neutrino Revolution

  17. Muon Flux state of art TAUP 13 Sept 13 DF in ERICE 23 September: Neutrino Revolution

  18. Atmospheric neutrino Pollution makes life impossible for other 18 neutrino • If among 28 events 10 are polluted muon or muon neutrino then: all 7 tracks are among these 10 atmospheric ones • Assuming an oscillated neutrino flavor 1:1:1 Not the relic 18 where most or all are electron or tau • The probability of the muon non appearence in 18 events is: 0.00067..if just one muon is extraterrestrial the probability is 0.1%... • Therefore IT IS MUCH BETTER TO IMAGINE ALMOST ALL neutrino as extra terrestrial: • But we need A SHARP CHANGE in spectra • Already from 100 keV energy.. DF in ERICE 23 September: Neutrino Revolution

  19. Neutrino first Summary:most no atmospheric, but extraterrestrial Arrival size: DF in ERICE 23 September: Neutrino Revolution

  20. the rarest Upward muon neutrino DF in ERICE 23 September: Neutrino Revolution

  21. The new sky map DF in ERICE 23 September: Neutrino Revolution

  22. The Map CONNECTION: Up dated ARGO Ricap Di Sciascio and ICECUBE Desiati 2013 ALL parallel TEV UHECR DF in ERICE 23 September: Neutrino Revolution

  23. DF in ERICE 23 September: Neutrino Revolution

  24. DF in ERICE 23 September: Neutrino Revolution

  25. The electron versus muon rate DF in ERICE 23 September: Neutrino Revolution

  26. The simplest the best:the exponential cut off at 100 keV DF in ERICE 23 September: Neutrino Revolution

  27. Possible approximations DF in ERICE 23 September: Neutrino Revolution

  28. The model that may better describe both electron and muon fluxes DF in ERICE 23 September: Neutrino Revolution

  29. DF in ERICE 23 September: Neutrino Revolution

  30. A Fermi Fountain shadows? DF in ERICE 23 September: Neutrino Revolution

  31. ANTARES signal over Fermi Fountain DF in ERICE 23 September: Neutrino Revolution

  32. DF in ERICE 23 September: Neutrino Revolution

  33. A THIRD PeV …neutrinoelectron again? Less than 4% to occur DF in ERICE 23 September: Neutrino Revolution

  34. Conclusions • We are seing a new Neutrino Astronomy • Puzzled by the flavor transition..Our solution assume already at 10 TeVs an extraterrestrial presence • The Galactic origin is favored by mild correlations in maps (UHECR,Neutrinos) • Extragalactic component may overcome CMB opacity and it may accumulate because a better visibility than gamma PeV photons; • Vela, Cygnus X3, Galactic Center maybe first sources • UHECR doublet correlation with W49B and W44 rises • Horizontal muon tracks conting may calibrate atmospheric neutrinos • Tau airshowers in horizons may see first airshowers DF in ERICE 23 September: Neutrino Revolution

  35. Thank you for theequinox attention DF in ERICE 23 September: Neutrino Revolution

  36. Daniele Fargion,D.D’armiento,P.Paggi, P.Desiati Beaming Neutrino across the Earth to test in Icecube neutrino mixing, and mass hierarchy. The Astrophysical Journal, 758:3 (15pp), 2012 October 10 DF in ERICE 23 September: Neutrino Revolution

  37. Inverted Hierarchi detection DF in ERICE 23 September: Neutrino Revolution

  38. Detection efficency DF in ERICE 23 September: Neutrino Revolution

  39. About Analemma • Exposures were made at the same time of day (9:00am local time), capturing the Sun's position on dates from January 7 through December 20, 2003. The multiple suns trace an intersecting curve known as an analemma. A foreground base exposure of the Temple of Apollo in ancient Corinth, Greece, appropriate for an analemma, was digitally merged with the film image. Equinox dates correspond to the middle points (not the intersection point) of the analemma. The curve is oriented at the corresponding direction and altitude for the temple, so the Sun's position for the September equinox is at the upper midpoint near picture center. Summer and winter solstices are at analemma top and bottom. DF in ERICE 23 September: Neutrino Revolution

  40. Possible changes in flavors DF in ERICE 23 September: Neutrino Revolution

  41. DF in ERICE 23 September: Neutrino Revolution

  42. The Map connecting UHECR and UHE neutrinos DF in ERICE 23 September: Neutrino Revolution

  43. Real volume size DF in ERICE 23 September: Neutrino Revolution

  44. Where is the answer? • If the extraterrestrial highest hundreds TeV neutrinos are also muons then, around the cubic km, muons must be born and they (if inclined or horizontal) must cross the detector at a rate of 20-40 each year: Just at horizons—they maybe a meter of flavor • The atmosphere and the Horizontal ice itself maybe source of horizontal.upgoing air-shower at a rate observable as Cherenkov lights in Antartic dark nights DF in ERICE 23 September: Neutrino Revolution

  45. Detection efficency DF in ERICE 23 September: Neutrino Revolution

More Related