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Theoretical dark matter halo kinematics and triaxial shape

Autor
Salvador, E.; Serra, S.; Manrique, A.; Gonzalez-Casado, G.
Tipus d'activitat
Article en revista
Revista
Monthly notices of the Royal Astronomical Society
Data de publicació
2012-08-21
Volum
424
Número
4
Pàgina inicial
3129
Pàgina final
3144
DOI
https://doi.org/10.1111/j.1365-2966.2012.21475.x Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/17510 Obrir en finestra nova
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 t...
Citació
Salvador-Solé, E. [et al.]. Theoretical dark matter halo kinematics and triaxial shape. "Monthly notices of the Royal Astronomical Society", 21 Agost 2012, vol. 424, núm. 4, p. 3129-3144.
Grup de recerca
gAGE - Grup d'Astronomia i Geomatica

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