Carregant...
Fitxers
Tipus de document
ArticleVersió
Versió publicadaData de publicació
Tots els drets reservats
Si us plau utilitzeu sempre aquest identificador per citar o enllaçar aquest document: https://hdl.handle.net/2445/192986
Theoretical dark matter halo kinematics and triaxial shape
Títol de la revista
Director/Tutor
ISSN de la revista
Títol del volum
Recurs relacionat
Resum
In a recent paper, Salvador-Solé et al. have derived the typical inner structure of dark matter haloes from that of peaks in the initial random Gaussian density field, determined by the power spectrum of density perturbations characterizing the hierarchical cosmology under consideration. In this paper, we extend this formalism to the typical kinematics and triaxial shape of haloes. Specifically, we establish the link between such halo properties and the power spectrum of density perturbations through the typical shape of peaks. The trends of the predicted typical halo shape, pseudo-phase-space density and anisotropy profiles are in good agreement with the results of numerical simulations. Our model sheds light on the origin of the power-law-like pseudo-phase-space density profile for virialized haloes.
Matèries (anglès)
Citació
Citació
SALVADOR SOLÉ, Eduard, SERRA, Sinue, MANRIQUE OLIVA, Alberto, GONZÁLEZ CASADO, Guillermo. Theoretical dark matter halo kinematics and triaxial shape. _Monthly Notices of the Royal Astronomical Society_. 2012. Vol. 424, núm. 4, pàgs. 3129-3144. [consulta: 27 de gener de 2026]. ISSN: 0035-8711. [Disponible a: https://hdl.handle.net/2445/192986]