23.05.2014 Views

neutrino

neutrino

neutrino

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

low energies, but it does not change the large discrepancies<br />

between our upward muon rates compared with Eq.<br />

(27) at energies closer to E µ ∼ m χ .<br />

10<br />

∫<br />

dN / dE µ<br />

(GeV -1 yr -1 )<br />

2<br />

1.5<br />

1<br />

0.5<br />

0<br />

m !<br />

= 500 GeV<br />

(Earth, upward)<br />

(Sun, upward)<br />

(Earth, contained)<br />

(Sun, contained)<br />

!! -> ""<br />

100 200 300 400 500<br />

E µ<br />

(GeV)<br />

whe<br />

give<br />

TeV<br />

In<br />

from<br />

2π s<br />

dom<br />

shap<br />

the<br />

trin<br />

mos<br />

from<br />

muo<br />

T<br />

mos<br />

the

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!