experiment X

experiment Xexperiment X

• ’ss per day :per day :

> 100 per day> 100 per day• total statistics :total statistics :

> 10> 1066 overover 10yr10yr• energy :energy :

0.1 ~ 10,000 TeV0.1 ~ 10,000 TeV

IceCube… 1 million IceCube… 1 million neutrinosneutrinos

• analytic IceCube simulation• TeV neutrinos oscillate, propagate, regenerate and decay… coherently

new physics signaturesunmatched sensitivity

Gonzalez-Garcia, Maltoni

your own IceCube simulation

# events = # events = ∫ Area Time Area Time {{ //

Input: A (EInput: A (E) from astro-ph/0305196) from astro-ph/0305196 Cuts:Cuts:

• length of muon track > 300 mlength of muon track > 300 m• number of channels as a function of zenith angle number of channels as a function of zenith angle

implemented as integration limits on the muonimplemented as integration limits on the muon range and energy as a function of zenithrange and energy as a function of zenith

Neutrinos

• oscillate• interact• regenerate • tau decay

new physics with atmospheric neutrinos

New Physics with the Atmospheric Beam

induced by new vector/tensor-like interactionsinduced by new vector/tensor-like interactions

withwith

New Physics with the Atmospheric Beam:

Examples•Violation of the equivalence principle:Violation of the equivalence principle:

•Violation of Lorentz invariance:Violation of Lorentz invariance:

new physics with atmospheric neutrinos

Total

455,246(10 years)

Or,Or,• zero mass eigenstates in vacuum• neutrino decay• neutrinos of varying mass•…..

Cosmic neutrino beam from the decay of pions

e e : : : : ~ 1 : 2 : <10 ~ 1 : 2 : <10-5-5 @ the source@ the source

e e : : : : ~ 1 : 1 : 1 @ the detector ~ 1 : 1 : 1 @ the detector

(maximal (maximal mixing) mixing)

TeV B L A Z A R 1ES 1959+650 a posteriori coincidence

H. Krawczynski et al, 2004ApJ,601 151K ‘Multiwavelength Observations of Strong Flares from the TeV Blazar 1ES 1959+650’

“orphan” flare

TeV Flux (Crab)

10 keV Flux (keV-1 cm-2 s-1)

PRELIMINARY

RadiationEnvelopingBlack Hole

Black Hole

p + -> n + +

~ cosmic ray + neutrino -> p + 0

~ cosmic ray + gamma

NEUTRINO BEAMS: HEAVEN & EARTHNeutrino Beams: Heaven & Earth

Neutrino Beams: Heaven & Earth

-rays from 0 decay discovered ?

∫ E N (E) = ∫ E N (E)

1 < < 8transparent transparent sourcesource

00 = = ++ = = -

acceleratorbeam dump(hidden source)

flux predicted observed -ray flux

~20 per km2 ~20 per km2 RX J1713-3946 RX J1713-3946 per year (galactic center)per year (galactic center)

HESS: RX J1713 HESS: RX J1713 SpectrumSpectrum

18 h 2003 data

Resolution ~10 arcmin

First resolved TeV image

energy conservation and cascadingenergy conservation and cascading

E-2.8

EE-2-2

m m 00

TeVTeV

Input: transparent source of 1 Crab with 2 < EInput: transparent source of 1 Crab with 2 < E < 20 TeV < 20 TeV

gamma ray slopegamma ray slope

2.8

2.5

2.2

1E 1959+6801E 1959+680