Visualization of Lyman-alpha radiative transfer on simulation boxes. Left to right: z=2.0,3.0,4.0,5.9.
Clustering Distortions from Lyman-alpha Radiative Transfer - A short introduction
Abstract
The dimensionally split power spectrum/two-point correlation are standard tools for constraining the cosmological model from redshift surveys. Given the Lyman-alpha emission line, I will try to motivate what significant distortions from the line’s radiative transfer modify those statistics.
Date
Apr 13, 2018 10:20 AM — 10:40 AM
Event
IMPRS Symposium Spring 2018
Location
Garching, Germany
For an easy explanation of this talk’s content, check this 10 minutes read or see this seminar talk (slides available).
Chris Byrohl
Postdoc
My research interests include cosmoslogical galaxy formation simulations, Lyman-$\alpha$ radiation to study galaxies and the large-scale structure, supernovae type Ia and high-performance computing.