P. Sikivie et al., SECONDARY INFALL MODEL OF GALACTIC HALO FORMATION AND THE SPECTRUM OFCOLD DARK-MATTER PARTICLES ON EARTH, Physical review. D. Particles and fields, 56(4), 1997, pp. 1863-1878
The spectrum of cold dark matter particles on Earth is expected to hav
e peaks in velocity space associated with particles which are falling
onto the Galaxy for the first time and with particles which have falle
n in and out of the Galaxy only a small number of times in the past. W
e obtain estimates for the velocity magnitudes and the local densities
of the particles in these peaks. To this end we use the secondary inf
all model of galactic halo formation which we have generalized to take
account of the angular momentum of the dark matter particles. The new
model is still spherically symmetric and it admits self-similar solut
ions. In the absence of angular momentum, the model produces flat rota
tion curves for a large range of values of a parameter epsilon which i
s related to the spectrum of primordial density perturbations. We find
that the presence of angular momentum produces an effective core radi
us; i.e., it makes the contribution of the halo to the rotation curve
go to zero at zero radius. The model provides a detailed description o
f the large scale properties of galactic halos including their density
profiles, their extent, and total mass. We obtain predictions for the
kinetic energies of the particles in the velocity peaks and estimates
for their local densities as functions of the amount of angular momen
tum, the age of the Universe, and epsilon.