Ref HAL: hal-00008561_v1
Ref Arxiv: astro-ph/0210149
Ref. & Cit.: NASA ADS
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Résumé:

We consider the observational constraints from the detection of antiprotons in the Galaxy on the amount of Primordial Black Holes (PBH) produced from primordial power spectra with a bumpy mass variance. Though essentially equivalent at the present time to the constraints from the diffuse $\\gamma$-ray background, they allow a widely independent approach and they should improve sensibly in the nearby future. We discuss the resulting constraints on inflationary parameters using a Broken Scale Invariance (BSI) model as a concrete example.

Commentaires: 10 pages, 3 figures