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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


PLANCK AND AUGER with TA ..from 55 EeV ICECUBE Desiati 2013

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 ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


Fermi gamma sources and uhecr
Fermi gamma sources and UHECR ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


Neutrino may day 13 madison usa 2 26 events
Neutrino May day 13 ICECUBE Desiati 2013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 events ICECUBE Desiati 2013Cascades 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 ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


Somehow the 28 are puzzling
Somehow the 28 are puzzling ICECUBE Desiati 2013

  • 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 ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution



The flavor sorpasso revolution
The Flavor ICECUBE Desiati 2013Sorpasso 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: ICECUBE Desiati 2013just 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 ICECUBE Desiati 2013

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


Neutrino first Summary: other 18 neutrinomost no atmospheric, but extraterrestrial

Arrival size:

DF in ERICE 23 September: Neutrino Revolution


The rarest upward muon neutrino
the rarest Upward muon neutrino other 18 neutrino

DF in ERICE 23 September: Neutrino Revolution


The new sky map
The new sky map other 18 neutrino

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 ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


The simplest the best the exponential cut off at 100 kev
The simplest the best: ICECUBE Desiati 2013the exponential cut off at 100 keV

DF in ERICE 23 September: Neutrino Revolution


Possible approximations
Possible approximations ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


The model that may better describe both electron and muon fluxes
The model that may better describe ICECUBE Desiati 2013both electron and muon fluxes

DF in ERICE 23 September: Neutrino Revolution



A fermi fountain shadows
A Fermi Fountain shadows? ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


ANTARES signal over Fermi Fountain ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution



A third pev neutrino electron again less than 4 to occur
A THIRD PeV …neutrino ICECUBE Desiati 2013electron again? Less than 4% to occur

DF in ERICE 23 September: Neutrino Revolution


Conclusions
Conclusions ICECUBE Desiati 2013

  • 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 the ICECUBE Desiati 2013equinox 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.Desiati ICECUBE Desiati 2013

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


Inverted hierarchi detection
Inverted Hierarchi detection ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


Detection efficency
Detection ICECUBE Desiati 2013efficency

DF in ERICE 23 September: Neutrino Revolution


About analemma
About Analemma ICECUBE Desiati 2013

  • 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 ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution



The Map connecting UHECR and UHE neutrinos ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


Real volume size
Real volume size ICECUBE Desiati 2013

DF in ERICE 23 September: Neutrino Revolution


Where is the answer
Where is the answer? ICECUBE Desiati 2013

  • 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 ICECUBE Desiati 2013efficency

DF in ERICE 23 September: Neutrino Revolution


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