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The clustering of dark matter, haloes & galaxies [PDF]
, 2008 In this thesis I study the spatial distribution of galaxies, haloes and dark matter particles using a suite of state-of-art cosmological N-body simulations of the growth structure in the Universe.
Angulo de la Fuente, Raúl Esteban
core
How do galaxies populate dark matter haloes? [PDF]
Monthly Notices of the Royal Astronomical Society, 2010 11 pages, 7 figures; revisions to both text and figures; matches version submitted to ...
Guo, Q. +3 more
openaire +3 more sources
Scalable Computation of Topological Abstractions for Scalar Data
Computer Graphics Forum, EarlyView.Abstract Topological data analysis has become an important tool for large scale scalar data analysis and visualization, efficiently extracting the inherent structure and features of interest of the data. However, with growing dataset sizes and complexity, it is increasingly becoming infeasible to compute topological abstractions of interest in serial ...
M. Will +6 more
wiley +1 more source
The Clustering of Dark Matter, Haloes & Galaxies [PDF]
, 2008 In this thesis I study the spatial distribution of galaxies, haloes and dark matter particlesin the Universe. The subjects investigated are conceptually divided into three areas.One line of research, which is made up of Chapters 2 and 3， is to explore ...
Raúl Esteban Angulo de la Puente,
core
Galaxy-Induced Transformation of Dark Matter Halos
, 2009 Fil: Babul, Arif.
Abadi, Mario Gabriel +4 more
openaire +3 more sources
Why Artificial Disruption Is Not a Concern for Current Cosmological Simulations
The Astrophysical JournalRecent studies suggest that cold dark matter subhalos are hard to disrupt and almost all cases of subhalo disruption observed in numerical simulations are due to numerical effects.
Feihong He, Jiaxin Han, Zhaozhou Li
doaj +1 more source
Survey on Visualization of Information Diffusion over Networks
Computer Graphics Forum, EarlyView.Abstract Information Diffusion (ID) describes how a value (e.g., a pathogen, a rumor, a packet) spreads through an underlying “medium” network of elements (e.g., a social or computer network). Understanding the information diffusion process is essential to predicting trends, controlling misinformation, and enhancing decision‐making as well as ...
T. Baumgartl +8 more
wiley +1 more source
Red Halos of Galaxies – Reservoirs of Baryonic Dark Matter? [PDF]
Proceedings of the International Astronomical Union, 2007 AbstractDeep optical/near-IR surface photometry of galaxies outside the Local Group have revealed faint and very red halos around objects as diverse as disk galaxies and starbursting dwarf galaxies. The colours of these structures are too extreme to be reconciled with stellar populations similar to those seen in the stellar halos of the Milky Way or ...
Zackrisson, E. +5 more
openaire +2 more sources
EDGE: the shape of dark matter haloes in the faintest galaxies
Monthly Notices of the Royal Astronomical Society, 2023 ABSTRACT Collisionless dark matter only (DMO) structure formation simulations predict that dark matter (DM) haloes are prolate in their centres and triaxial towards their outskirts. The addition of gas condensation transforms the central DM shape to be rounder and more oblate.
Matthew D A Orkney +7 more
openaire +6 more sources
Self-similar Decomposition of the Hierarchical Merger Tree of Dark Matter Halos
The Astrophysical JournalIn the ΛCDM universe, structure formation is generally not a self-similar process, while some self-similarity remains in certain statistics, which can greatly simplify our description and understanding of the cosmic structures. In this work, we show that
Wenkang Jiang +3 more
doaj +1 more source