The lcdm model at small scalesMilky way satellites and cusp-core crisis

  1. Di Cintio , Arianna
unter der Leitung von:
  1. Alexander Knebe Doktorvater/Doktormutter
  2. Alessandro Melchiorri Co-Doktorvater/Doktormutter

Universität der Verteidigung: Universidad Autónoma de Madrid

Fecha de defensa: 21 von Juli von 2014

Gericht:
  1. Rosa Domínguez Tenreiro Präsident/in
  2. Stefan Gottloeber Sekretär/in
  3. Antonio López Maroto Vocal
  4. Carlos Muñoz López Vocal
  5. Marco De Petris Vocal

Art: Dissertation

Teseo: 378148 DIALNET

Zusammenfassung

Cosmology-the study of the formation and ultimate fate of structures and galaxies throughout the Universe- is without a doubt one of the most exciting fields in astrophysics today. Over the last twenty years a picture has emerged in which contemporary structures (e.g. galaxies, galaxy groups and clusters, and the filamentary network in-between) have evolved by gravitational amplification of seed inhomogeneities that are likely of quantum origin and were produced shortly after the Big Bang. This picture ties together (observational) measurements of the cosmic background radiation, estimastes of the primordial abundances of the light elements measurements of the clustering of galaxies and, to a more limited extent, the characteristic properties of individual galaxies. (Parte del Informe del Dr. D. Alexander Knebe)