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- W1567338308 abstract "We derive the density profile of cold dark matter halos using a self-similar accretion model. We show that if the clumpiness of the infalling matter is taken into account, then the inner density slope, d(log{rho})/d(log{r}), is close to -1. Compared with the density profiles predicted by different numerical simulations, we find that outside ~0.1% of the virial radius, our solutions agree best with the fitting formula proposed by Navarro et al. (2004), d(ln{rho})/d(ln{r})=-2(r/R)^0.17, where R is a characteristic radius, inside which the density profile becomes shallower than isothermal." @default.
- W1567338308 created "2016-06-24" @default.
- W1567338308 creator A5063402054 @default.
- W1567338308 date "2006-08-29" @default.
- W1567338308 modified "2023-09-27" @default.
- W1567338308 title "The structure of dark matter halos: self-similar models versus N-body simulations" @default.
- W1567338308 hasPublicationYear "2006" @default.
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