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Дата индексирования: Sat Feb 12 13:09:11 2011
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Поисковые слова: m 8

"I have done a terrible thing. I have postulated a particle that cannot be detected" Wolfgang Pauli

.

.. .M. ..

-2010 « » ,






2*1020 s 7 TeV LHC = 00 14 , 8*1016 eV




2*1020 s 7 TeV LHC = 00 14 , 8*1016 eV



mv<1
"TeV Strings and the Neutrino-Nucleon Cross Section at Ultra-high Energies", F. Cornet, arXiv:hepph/0102065

5 - 5%



+ + + +

CMB CMB CMB CMB

+ + + + e- + e l +W
± +

=10 =10 =10

-66

m

-2

,
-2

-52

m m
-34

-2

-47

-2

=8·10

m





Top-down:


Bottom-up:



"X" > : - GZK- , , -


1-10




GZK

­ - (GZK) cutoff at 6*1019 Lint < 50

p +

CM B

n +

+

n + p +

-

± µ ± +
p + p +
0

µ µ

µ ± e ± + e +
CM B

0 +
p + p ±0 K ± D
±0

decay

+

CM B

µ+ + µ

-

µ e + e +
412

µ

cmb



-

p +

CM B

e- + e+ + p

scattering



!

GZK-v =1019 ­ 5 \2\ 1020 - 1 \2\100

7










Baikal ANTARES NEMO NESTOR (KM3Net)

IceCube ANTARES IceCube

EUSO PAO O WL

RESUN ANITA GLINT LORD Astropeiler NuMoon GMRT RICE S al S a ARIANNA AR A LunaSKA LOFAR




1965

+ e-at + ee+ + e-at e+ + ee- + e-at e- + ee+ + e-at +

~ ~
1 - 18 m - 1 km

1.5 ~ 10 ~3 2 -6

"Coherent Radio Emission from Cosmic Showers in Air and in Dense Media", Askar'yan, G. A., Soviet Physics JETP, Vol.



1965 , 2000 SLAC


RAMAND


RICE

ARA

Sa l Sa ANITA AURA ARIANN A
Cosmic rays are protons

"Radio Detection of GZK Neutrinos - AURA status and plans", H. Landsman etc, Proceedings of the 30th International Cosmic Ray Conference, Vol. 4, p827­830 "Simulation of the Event Reconstruction of Ultra High Energy Cosmic Neutrinos with Askaryan Radio Array", Shang-Yu Sun, Pisin Chen and Melin Huang, 2010,







GLUE
2004

Kalyazin 2005

Parkes 2007

NuMoon

GMRT

GLINT RESUN

LOFAR LunaSKA (ATCA)






(...)
3

- V

eff

~ 10

5








-



SN1987 A

Markarian 501 136 Mpc 1013 eV Lint ~ 70 Mpc


!
. . .. .. ..




-2010 « » ,