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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.

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revolution within icecube horizons
Revolution within ICECUBE Horizons

DF in ERICE 23 September: Neutrino Revolution

gamma neutrino uhecr in sky

Icecube

2013

AUGER

GZK

Gamma-Neutrino-UHECR in sky

DF in ERICE 23 September: Neutrino Revolution

the map connection up dated argo ricap di sciascio and icecube desiati 2013
The Map CONNECTION: Up dated ARGO Ricap Di Sciascio and ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution

slide4

PLANCK AND AUGER with TA ..from 55 EeV

DF in ERICE 23 September: Neutrino Revolution

last ta and auger and multiplet events at 20 eev
Last TA and AUGER and Multiplet events at 20 EeV

DF in ERICE 23 September: Neutrino Revolution

fermi gamma sources and uhecr
Fermi gamma sources and UHECR

DF in ERICE 23 September: Neutrino Revolution

neutrino may day 13 madison usa 2 26 events
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

horizontal or inclined events cascades and tracks
Horizontal or inclined eventsCascades and tracks

DF in ERICE 23 September: Neutrino Revolution

showering versus tracks tau are sphere cascades below pev
Showering versus tracks: tau are sphere cascades below PeV

DF in ERICE 23 September: Neutrino Revolution

somehow the 28 are puzzling
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

where we are looking in the flux map of the universe
Where we are looking in the flux map of the universe

DF in ERICE 23 September: Neutrino Revolution

the flavor sorpasso revolution
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

expected flux a year ago 2012 just eev gzk neutrino no pev ones
Expected flux a year ago 2012: just EeV GZK neutrino, no PeV ones

DF in ERICE 23 September: Neutrino Revolution

muon flux state of art taup 13 sept 13
Muon Flux state of art TAUP 13 Sept 13

DF in ERICE 23 September: Neutrino Revolution

atmospheric neutrino pollution makes life impossible for other 18 neutrino
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

slide19

Neutrino first Summary:most no atmospheric, but extraterrestrial

Arrival size:

DF in ERICE 23 September: Neutrino Revolution

the rarest upward muon neutrino
the rarest Upward muon neutrino

DF in ERICE 23 September: Neutrino Revolution

the new sky map
The new sky map

DF in ERICE 23 September: Neutrino Revolution

the map connection up dated argo ricap di sciascio and icecube desiati 20131
The Map CONNECTION: Up dated ARGO Ricap Di Sciascio and ICECUBE Desiati 2013

ALL parallel TEV UHECR

DF in ERICE 23 September: Neutrino Revolution

the electron versus muon rate
The electron versus muon rate

DF in ERICE 23 September: Neutrino Revolution

the simplest the best the exponential cut off at 100 kev
The simplest the best:the exponential cut off at 100 keV

DF in ERICE 23 September: Neutrino Revolution

possible approximations
Possible approximations

DF in ERICE 23 September: Neutrino Revolution

the model that may better describe both electron and muon fluxes
The model that may better describe both electron and muon fluxes

DF in ERICE 23 September: Neutrino Revolution

a fermi fountain shadows
A Fermi Fountain shadows?

DF in ERICE 23 September: Neutrino Revolution

slide31

ANTARES signal over Fermi Fountain

DF in ERICE 23 September: Neutrino Revolution

a third pev neutrino electron again less than 4 to occur
A THIRD PeV …neutrinoelectron again? Less than 4% to occur

DF in ERICE 23 September: Neutrino Revolution

conclusions
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

thank you for the equinox attention
Thank you for theequinox attention

DF in ERICE 23 September: Neutrino Revolution

daniele fargion d d armiento p paggi p desiati
Daniele Fargion,D.D’armiento,P.Paggi, P.DesiatiBeaming 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

inverted hierarchi detection
Inverted Hierarchi detection

DF in ERICE 23 September: Neutrino Revolution

detection efficency
Detection efficency

DF in ERICE 23 September: Neutrino Revolution

about analemma
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

possible changes in flavors
Possible changes in flavors

DF in ERICE 23 September: Neutrino Revolution

slide42

The Map connecting UHECR and UHE neutrinos

DF in ERICE 23 September: Neutrino Revolution

real volume size
Real volume size

DF in ERICE 23 September: Neutrino Revolution

where is the answer
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

detection efficency1
Detection efficency

DF in ERICE 23 September: Neutrino Revolution

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