No Observational Constraints from Hypothetical Collisions of Hypothetical Dark Halo Primordial Black Holes with Galactic Objects
Artikel i vetenskaplig tidskrift, 2009

It was suggested by several authors that hypothetical primordial black holes (PBHs) may contribute to the dark matter (DM) in our Galaxy. There are strong constraints based on the Hawking evaporation that practically exclude PBHs with masses m pbh ~ 1015to1016 g and smaller as significant contributors to the Galactic DM. Similarly, PBHs with masses greater than about 1026 g are practically excluded by the gravitational lensing observation. The mass range between 1016 g

early universe

dark matter

X-rays: bursts

Galaxy: abundances

gamma rays: bursts


Marek A Abramowicz

Göteborgs universitet

Julia K. Becker

Ruhr-Universität Bochum

Göteborgs universitet

Peter L. Biermann

Karlsruher Institut für Technologie (KIT)

Universität Bonn

Max Planck-institutet

University of Alabama

Antonella Garzilli

Göteborgs universitet

Scuola Internazionale Superiore di Studi Avanzati

Fredrik Johansson

Göteborgs universitet

Chalmers, Fundamental fysik

Lei Qian

Peking University

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 705 1 659-669





Mer information

Senast uppdaterat