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UHE CR

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(1)

UHE CR

and

The GZK

Suppression

(2)

Ultra High Energy

Cosmic Rays (E > 1019 eV)

Energy Loss Mechanisms for of High Energy Particles

Interactions on the photons of the Microwave Cosmic Background (2.7 oK background)

(3)

Energy Loss Mechanisms

Redshift 

PhotoProduction Pair Production

Photo Disintegration

(4)

Cosmic  (2.7 K) Background Radiation 

Stellar Light Stellar Light

 reprocessed by dust

Average Photon Density in the Universe

(5)

Threshold for photoproduction:

Is determined by the threshold for pion production

(6)

The Greisen ­Zatsepin­Kuzmin  “cutoff” 

Photoproduction   Threshold

cos e = -1

(7)

)

)

Energy Loss in one interaction

At threshold:

The pion and the proton are produced at rest in the center of mass frame,

therefore they have the same velocity (and the same Lorentz Factor)

(8)

Laboratory (Proton Rest) Frame 

General Frame 

Ep

2Epmp>= (mp+m)2

(9)

Computation of the Absorption Length of a proton in the intergalactic photon Field.

Peak ++ at  ~300 MeV

(10)

Qualitative analyisis

(11)
(12)

Log 10[E (eV)]

Size of the visible Universe

GZK on CMB

GZK on all 

(13)

Effect of Pair Production interactions The threshold is lower

The cross section is higher

The energy loss per interaction is smaller Photoproduction of pions

Pair production

(14)
(15)

Absorption of High Energy Photons Center of mass cross section

(16)

Inverse of absorption length for pair creation

(17)

Absorption for extragalactoc sources in Cherenkov Telescopes (TeV) is important

Due to starlight where there is high uncertainties

(18)

Propagation of Nuclei

(19)

Discrepancy

between the two largest  experiments

AGASA

HIRES

(20)
(21)
(22)

Structure in the Spectrum

Density of Cosmic Rays at the Present Epoch

Homogeneous Universe

Injection Rate

at the epoch t

Energy Loss

S0 (E0) * f (t) S0 (E0) * f (z)

(23)
(24)
(25)

Magnetic  Deviation

d

(26)
(27)

Models for the UHECR

BOTTOM­UP    (Acceleration of particles)   Active Galactic Nuclei

  Gamma Ray Bursts   ...

TOP­DOWN 

 

  (Decay of Massive Objects)    Topological Defects

   Super­Massive Particles ­ Wimpzillas

(28)

Absence of Cutoff :

Neutrinos 

 with anomalous large cross section

New Particles 

Z­burst Model   

(“Neutrino Carrier”)

VIOLATIONS  of LORENTZ  INVARIANCE 

Excess of Nearby Sources 

(29)

WIMPZILLA's

M = 109  ­ 1019 GeV 

(30)

TOP - DOWN Models

High Energy Cosmic Rays as DECAY products of

Massive "Exotic" Objects (Relics of the Early Universe) Topological Defects. SuperMassive Particles

(31)

Phenomenology of QUANTUM GRAVITY ?!

Effective speed of photons in quantum space foam

High Energy Photons delayed

(32)
(33)

Modifications  of  Reaction Thresholds

(34)

      AUGER detector  

(35)

      AUGER expectations: GZK  

(36)

      AUGER results: GZK  

(37)

      AUGER results:  and   

(38)

AUGER results: anisotropy

(39)

AUGER results: composition

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