FORMATION AND EVOLUTION OF SELF-INTERACTING DARK MATTER HALOS |
AHN KYUNGJIN
(Department of Astronomy, University of Texas)
SHAPIRO PAUL R. (Department of Astronomy, University of Texas) |
1 |
A Numerical Method for the Study of the Gravothermal Instability in Star Clusters
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DOI |
2 |
Self-Similar Gravitational Collapse in an Expanding Universe
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DOI |
3 |
Cold Collapse and the core Catastrophe
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DOI ScienceOn |
4 |
A Model for the Post-Collapse Equilibrium of Cosmological Structure: Truncated Isothermal Spheres from Top-Hat Density Perturbations
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DOI ScienceOn |
5 |
Collisional Dark Matter and the Structure of Dark Halos
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DOI |
6 |
Self-Similar Secondary Infall and Accretion in an Einstein-de Sitter Universe
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DOI |
7 |
Local Density Maxima - Progenitors of Structure
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DOI |
8 |
Collisional versus collisionless Dark Matter
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DOI |
9 |
Observational Evidence for Self-Interactiing Cold Dark Matter
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DOI ScienceOn |
10 |
Weakly Self-Interacting Dark Matter and the Structure of Dark Halos
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DOI ScienceOn |
11 |
The Structure and Evolution of Weakly Self-interacting Cold Dark Matter Halos
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DOI |
12 |
A Quantitative Study of Interacting Dark Matter in Halos
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DOI ScienceOn |
13 |
Halo Properties in Cosmological Simulations of Self-interacting Cold Dark Matter
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DOI ScienceOn |
14 |
Self-Interacting Dark Matter Halos and the Gravothermal Catastrophe
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DOI ScienceOn |
15 |
A Universal Density Profile from Hierarchical Clustering
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DOI ScienceOn |
16 |
Concentrations of Dark Halos from Their Assembly Histories
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DOI ScienceOn |