scholarly journals NIHAO project II: halo shape, phase-space density and velocity distribution of dark matter in galaxy formation simulations

2016 ◽  
Vol 462 (1) ◽  
pp. 663-680 ◽  
Author(s):  
Iryna Butsky ◽  
Andrea V. Macciò ◽  
Aaron A. Dutton ◽  
Liang Wang ◽  
Aura Obreja ◽  
...  
2011 ◽  
Vol 415 (4) ◽  
pp. 3895-3902 ◽  
Author(s):  
Aaron D. Ludlow ◽  
Julio F. Navarro ◽  
Simon D. M. White ◽  
Michael Boylan-Kolchin ◽  
Volker Springel ◽  
...  

2013 ◽  
Vol 430 (3) ◽  
pp. 2346-2357 ◽  
Author(s):  
Shi Shao ◽  
Liang Gao ◽  
Tom Theuns ◽  
Carlos S. Frenk

2009 ◽  
Vol 395 (3) ◽  
pp. 1225-1236 ◽  
Author(s):  
Ileana M. Vass ◽  
Monica Valluri ◽  
Andrey V. Kravtsov ◽  
Stelios Kazantzidis

2009 ◽  
Vol 18 (03) ◽  
pp. 477-484
Author(s):  
DING MA ◽  
PING HE

N-body simulations of dark matter halos show that the density profiles of the halos behave as ρ(r) ∝ r-α(r), where the density logarithmic slope α ≃ 1–1.5 in the center and α ≃ 3–4 in the outer parts of the halos. However, some observations are not in agreement with simulations in the very central region of the halos. The simulations also show that the velocity dispersion anisotropy parameter β ≈ 0 in the inner part of the halo and the so-called pseudo–phase-space density ρ/σ3 behaves as a power law in radius r. With these results in mind, we study the distribution function and the pseudo–phase-space density ρ/σ3 of the center of dark matter halos and find that they are closely related.


2009 ◽  
Vol 698 (2) ◽  
pp. 1813-1825 ◽  
Author(s):  
Ileana M. Vass ◽  
Stelios Kazanzidis ◽  
Monica Valluri ◽  
Andrey V. Kravtsov

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