Hahn, Olivier
Oliver Hahn Physiker und Hochschullehrer (1977- )
Hahn, Oliver 1977-
VIAF ID: 202109696 (Personal)
Permalink: http://viaf.org/viaf/202109696
Preferred Forms
- 100 1 _ ‡a Hahn, Oliver ‡d 1977-
- 100 1 _ ‡a Hahn, Olivier
- 100 1 _ ‡a Hahn, Olivier
- 100 0 _ ‡a Oliver Hahn ‡c Physiker und Hochschullehrer (1977- )
4xx's: Alternate Name Forms (3)
5xx's: Related Names (4)
- 551 _ _ ‡a Tübingen ‡4 ortw ‡4 https://d-nb.info/standards/elementset/gnd#placeOfActivity
- 510 2 _ ‡a Universität Wien ‡b Fakultät für Mathematik ‡4 affi ‡4 https://d-nb.info/standards/elementset/gnd#affiliation ‡e Affiliation
- 510 2 _ ‡a Universität Wien ‡b Institut für Astrophysik ‡4 affi ‡4 https://d-nb.info/standards/elementset/gnd#affiliation ‡e Affiliation
- 551 _ _ ‡a Zürich ‡4 ortw ‡4 https://d-nb.info/standards/elementset/gnd#placeOfActivity
Works
Title | Sources |
---|---|
An adaptively refined phase–space element method for cosmological simulations and collisionless dynamics | |
Ageing-associated small RNA cargo of extracellular vesicles | |
The AGORA high-resolution galaxy simulations comparison project | |
Analytical growth functions for cosmic structures in a ΛCDM Universe | |
The anisotropic two-point correlation functions of the nonlinear traceless tidal field in the principal-axis frame | |
The Aspen–Amsterdam void finder comparison project | |
The buildup of the Hubble sequence in the cosmos field | |
Disruption of dark matter substructure: fact or fiction? | |
Earth-mass haloes and the emergence of NFW density profiles | |
ENZO: an adaptive mesh refinement code for astrophysics | |
The evolution of dark matter halo properties in clusters, filaments, sheets and voids | |
Four phases of angular-momentum buildup in high-z galaxies: from cosmic-web streams through an extended ring to disc and bulge | |
Halo-to-halo similarity and scatter in the velocity distribution of dark matter | |
How closely do baryons follow dark matter on large scales? | |
Lagrangian statistics of dark halos in a {Lambda}CDM cosmology | |
The large-scale orientations of disc galaxies | |
The locations of halo formation and the peaks formalism | |
Mergers and mass accretion for infalling halos both end well outside cluster virial radii | |
Multi-scale initial conditions for cosmological simulations | |
A new approach to simulating collisionless dark matter fluids | |
Place de la radiologie dans le bilan des testicules non palpables : à propos de 18 observations | |
Population III star formation in large cosmological volumes. I. Halo temporal and physical environment | |
The properties of cosmic velocity fields | |
Rhapsody-G simulations: galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxies | |
Rhapsody. II. Subhalo properties and the impact of tidal stripping from a statistical sample of cluster-size halos | |
Sources radio diffuses dans les amas de galaxies | |
Substructure and merger detection in resolved NIKA Sunyaev-Zel’dovich images of distant clusters | |
Tidal effects and the environment dependence of halo assembly | |
Tracing the cosmic web | |
Tracing the dark matter sheet in phase space | |
Two is better than one: joint statistics of density and velocity in concentric spheres as a cosmological probe | |
Virial scaling of galaxies in clusters: bright to faint is cool to hot | |
The warm dark matter halo mass function below the cut-off scale | |
What sets the central structure of dark matter haloes? |