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On Planetary-Mass Compact Objects as Dark Matter

Published online by Cambridge University Press:  26 May 2016

Erik Zackrisson,
Carina Persson and
Nils Bergvall
Erik Zackrisson
Affiliation:
Uppsala Astronomical Observatory, Box 515, SE 751 20 Uppsala, Sweden
Carina Persson
Affiliation:
Uppsala Astronomical Observatory, Box 515, SE 751 20 Uppsala, Sweden
Nils Bergvall
Affiliation:
Uppsala Astronomical Observatory, Box 515, SE 751 20 Uppsala, Sweden

Abstract

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We assess to what extent the claimed signature of planetarymass compact objects in the long-term optical light curves of quasars really can be explained by the dark matter populations allowed in the currently favoured ΩM = 0.3, ΩΛ = 0.7 cosmology. Revised upper limits on the cosmological density of planetary-mass compact objects inferred from the statistics of quasar light curves and the equivalent widths of quasar emission lines are also presented.

Information

Type
Part 4: Lensing
Information
Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004, pp. 133 - 134
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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