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2010

Comment on Calculation of Positron Flux from Galactic Dark Matter

Perelstein, Maxim, Shakya, Bibhushan

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Energetic positrons produced in annihilation or decay of dark matter particles in the Milky Way can serve as an important indirect signature of dark matter.

Computing the positron flux expected in a given dark matter model involves solving transport equations, which account for interaction of positrons with matter and galactic magnetic fields.
Existing calculations solve the equations inside the diffusion zone, where galactic magnetic fields confine positrons, and assume vanishing positron density on the boundaries of this zone.
However, in many models, a substantial fraction of the dark matter halo lies outside the diffusion zone.

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