Cosmology with Large-Scale Structure - Lecture 1
International Centre for Theoretical Sciences via YouTube
Overview
Syllabus
Large-scale structure as a cosmological probe
What we learn from LSS
Lecture plan
Statistical approach: Poisson clustering hypothesis
Bias: relating mass and light
Models for bias
High-peak bias
Testing the biased CDM linear P(k)
Projected clustering
1990: APM angular correlations, w(e)
Weighing the universe with horizons
The argument for A: 1990 LSS + CMB
Taught by
International Centre for Theoretical Sciences