2004/06/22 by R. Schild, Rudolph E. Schild, Schild, R.
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0406491
Review for the Dark Matter/Dark Energy 2004 Conference at UCLA. 7 pages, no illustrations, but many references to published figures
arxiv created 2004/06/22 · openalex publication_date 2004/06/22 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Since the original baryonic dark matter detection from quasar microlensing was first announced in 1996, substantial strides have been made in confirming the rapid microlensing signature in the Q0957 system and in other gravitational lens systems. The most rapid event recognized had a 1% amplitude and a 12-hour duration. Interpretation of the rapid fluctuations has centered upon 3 offered explanations; microlensing of fine quasar structure by a population of planet mass astronomical bodies in the lens galaxy, orbiting bright structures in the accretion disc of the supermassive black hole of the quasar, or dark clouds swarming around the luminous quasar source. The observations, particularly the equal positive and negative fluctuations, seem to strongly favor the cosmological population of planetary mass objects in the lens galaxy. Of the several ideas advanced for the origin of such a population, the most appealing seems to be their birth at the time of recombination 300,000 years after the Big Bang.