Forgot your password?
A Clash of Clusters Provides New Clue to Dark Matter
Document Actions
Reionization and its Observational Consequences
Up one levelWe use N-body and radiative transfer simulations to model the reionization of the universe on scales of hundreds of comoving megaparsecs
- The radiative transfer method
- A brief introduction to our radiative transfer algorithm
- HI/HII region size distribution code
- A simple code for calculating HI/HII region size distribution from ionization field on a uniform cubic mesh
MASS: Lance Simms