Life after death: black hole evaporation in the Planck region

Details Life after death: black hole evaporation in the Planck region Life after death: black hole evaporation in the Planck region

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..401b&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

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Scientific paper

Primordial Black Holes may have formed in the early universe either from initial inhomogeneities or from phase transitions. Their possible detection by the emission of antiproton thanks to Hawking evaporation is very promising since new experimental data are available (BESS) and will be obtained in the years to come (AMS). On the other hand, theoretical works show that some fundamental parameters of string gravity could also be constrained by the residual emission of such objects.

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