A possible explanation for the electron/positron excess of ATIC/PAMELA

Details A possible explanation for the electron/positron excess of ATIC/PAMELA A possible explanation for the electron/positron excess of ATIC/PAMELA

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010raa....10...39y&link_type=abstract

Research in Astronomy and Astrophysics, Volume 10, Issue 1, pp. 39-46 (2010).

Astronomy and Astrophysics

Astrophysics

Scientific paper

Results from PAMELA and ATIC indicate that the Kaluza-Klein type dark matter particles could be the annihilation source of the observed excess of electrons and positrons. Assuming the existence of a nearby black hole with 10000-100000 solar masses and a point source boost algorithm, we apply the standard propagation model and find that the results fit the data well.

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