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We derive the strongest constraint on the fraction of dark matter that can be composed of low mass primordial black holes by using the observation of the Galactic Center 511 keV gamma-ray line.
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J. Knodlseder et al., The All-sky distribution of 511 keV electron-positron annihilation emission
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2006
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T. Totani, A RIAF Interpretation for the Past Higher Activity of the Galactic Center Black Hole and the 511-keV Annihilation Emission
2006
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W. Wang, C. S. J. Pun, and K. S. Cheng, Could electron-positron annihilation lines in the galactic center result from pulsar winds?
2006
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A. C. Cummings, E. C. Stone, B. C. Heikkila, N. Lal, W. R. Webber, G. Jóhannesson, I. V. Moskalenko, E. Orlando, and T. A. Porter, Galactic Cosmic Rays in the Local Interstellar Medium: Voyager 1 Observations and Model Results
2016
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2016
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2016
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E. G. Speckhard et al., Dark Matter Velocity Spectroscopy
2016
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N. Prantzos, On the intensity and spatial morphology of the 511-kev emission in the milky way
2006
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J. F. Beacom and H. Yuksel, Stringent constraint on galactic positron production
2006
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T. Matsuda, Primordial black holes from cosmic necklaces
2006
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G. Weidenspointner et al., An asymmetric distribution of positrons in the Galactic disk revealed by gamma-rays
2008
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2009
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2016
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F. Kuhnel and K. Freese, Constraints on Primordial Black Holes with Extended Mass Functions
2017
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F. H. Panther, Positron Transport and Annihilation in the Galactic Bulge
2018
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S. Pi, Y.-l. Zhang, Q.-G. Huang, and M. Sasaki, Scalaron from R 2 R^{2} -gravity as a heavy field
2018
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2018
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2018
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2019
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