On Planetary-Mass Compact Objects as Dark Matter

Details On Planetary-Mass Compact Objects as Dark Matter On Planetary-Mass Compact Objects as Dark Matter

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..220..133z&link_type=abstract

International Astronomical Union Symposium no. 220, held 21 - 25 July, 2003 in Sydney, Australia. Eds: S. D. Ryder, D. J. Pisano

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We assess to what extent the claimed signature of planetary-mass 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.

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