Self interactive dark matter in large scale structure
Magíster en Ciencias, Mención Astronomía === Cold Dark matter (ΛCDM) models have been remarkably successful to explain the observed large scale structure of our universe on scales of the order of galaxy clusters (≥ 4 Mpc) and above (therefore in this work we consider large scale beyond the aforeme...
Main Author: | Rincón Rivero, Ángel |
---|---|
Other Authors: | Palma Quilodrán, Gonzalo |
Language: | en |
Published: |
Universidad de Chile
2016
|
Subjects: | |
Online Access: | http://repositorio.uchile.cl/handle/2250/138441 |
Similar Items
-
Dark matter in a 'Z IND. 3'-symmetry extension of the Standard model
by: Koerich, Luan Vinícius [UNESP]
Published: (2018) -
Dark matter in a 'Z IND. 3'-symmetry extension of the Standard model /
by: Koerich, Luan Vinícius.
Published: (2015) -
Interacting dark energy models in Cosmology and large-scale structure observational tests
by: Rafael José França Marcondes
Published: (2016) -
Interacting dark energy models in Cosmology and large-scale structure observational tests
by: Marcondes, Rafael José França
Published: (2016) -
Cosmología hoy: una revisión
by: Jorge L Cervantes Cota, et al.
Published: (2007-09-01)