Andreas Faltenbacher (Cape Town)

Anisotropy in the matter distribution at very large scales
When Feb 27, 2012 from 02:00 PM to 03:00 PM
  • Colloquium
Where SH, Lecture hall
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Tracing the  cosmic evolution  of the Baryonic  Acoustic Oscillation (BAO) scale with galaxy two point correlation functions is currently the most promising approach to detect dark energy at early times.  A number of ongoing  and future experiments will measure the BAO peak with unprecedented accuracy.  N-body simulations indicate that the matter distribution  is  anisotropic out  to ~150 Mpc, far beyond the  BAO scale  of about 100 Mpc. I will discuss implications for the measurement of the BAO.