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Ultracompact minihalos have recently been proposed as a new class of dark matter structure.
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Ricotti & Gould [ 7 ] also discuss ultracompact minihalos containing PBHs, but these require similar amplitude density perturbations as PBHs, so are less appealing
Cited in the paper.
Using e.g. z = 30 z=30 instead has little impact on results
Cited in the paper.
http://fermi.gsfc.nasa.gov/ssc/data/analysis/documentation/Cicerone/Cicerone_LAT_IRFs/LAT_sensitivity.html
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The sensitivities in Fig. 1
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