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Gamma-ray Signal from Earth-mass Dark Matter Microhalos

  • Authors: Tomoaki Ishiyama, Junichiro Makino, and Toshikazu Ebisuzaki

ISHIYAMA, MAKINO, & EBISUZAKI 2010 The Astrophysical Journal Letters 723 L195.

  • Provider: AAS Journals

Caption: Figure 1.

Top and bottom panels show the distribution of dark matter at z = 31 for our standard model (A) and model without free-streaming cutoff (B). The width of the images corresponds to 12 comoving pc. Images in the squares are enlargements of single halos. The size of the squares is 0.6 comoving pc (4900 AU in physical units).

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