Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2009-01-22
Physics
High Energy Physics
High Energy Physics - Phenomenology
9 pages, 4 figures, 2 references added
Scientific paper
We study the spectrum of cosmic ray positrons produced by a scaling distribution of non-superconducting cosmic strings. In this scenario, the positrons are produced from the jets which form from the cosmic string cusp annihilation process. The spectral shape is a robust feature of our scenario, and is in good agreement with the results from the recent PAMELA and ATIC experiments. In particular, the model predicts a sharp upper cutoff in the spectrum, and a flux which rises as the upper cutoff is approached. The energy at which the flux peaks is determined by the initial jet energy. The amplitude of the flux can be adjusted by changing the cosmic string tension and also depends on the cusp annihilation efficiency.
Brandenberger Robert
Cai Yi-Fu
Xue Weimin
Zhang Xinmin
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