and Cosmology
Extragalactic Astronomy and Cosmology: An Introduction
Extragalactic Astronomy and Cosmology: An Introduction
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8. <strong>Cosmology</strong> III: The Cosmological Parameters<br />
316<br />
for red galaxies is larger by about a factor 1.4 than for<br />
blue galaxies. This result is not completely unexpected,<br />
because red galaxies are located preferentially in clusters<br />
of galaxies, whereas blue galaxies are rarely found<br />
in massive clusters. Hence, red galaxies seem to follow<br />
the density concentrations of the dark matter much<br />
more closely than blue galaxies.<br />
8.1.4 Effect of Peculiar Velocities<br />
Redshift Space. The relative velocities of galaxies in<br />
the Universe are not only due to the Hubble expansion<br />
but, in addition, galaxies have peculiar velocities. The<br />
peculiar velocity of the Milky Way is measurable from<br />
the CMB dipole (see Fig. 1.17). Owing to these peculiar<br />
velocities, the observed redshift of a source is the<br />
superposition of the cosmic expansion velocity <strong>and</strong> its<br />
peculiar velocity v along the line-of-sight,<br />
cz= H 0 D + v. (8.6)<br />
The measurement of the other two spatial coordinates<br />
(the angular position on the sky) is not affected by<br />
the peculiar velocity. The peculiar velocity therefore<br />
causes a distortion of galaxy positions in wedge diagrams,<br />
yielding a shift in the radial direction relative to<br />
their true positions. Since, in general, only the redshift<br />
is measurable <strong>and</strong> not the true distance D, the observed<br />
three-dimensional position of a source is specified by<br />
the angular coordinates <strong>and</strong> the redshift distance<br />
s = cz<br />
H 0<br />
= D + v H 0<br />
. (8.7)<br />
The space that is spanned by these three coordinates<br />
is called redshift space. In particular, we expect that<br />
the correlation function of galaxies is not isotropic in<br />
redshift space.<br />
Galaxy Distribution in Redshift Space. The best<br />
known example of this effect is the “Fingers of God”. To<br />
underst<strong>and</strong> their origin, we consider galaxies in a cluster.<br />
They are situated in a small region in space, all at<br />
roughly the same distance D <strong>and</strong> within a small solid<br />
angle on the sphere. However, due to the high velocity<br />
dispersion, the galaxies span a broad range in s,<br />
which is easily identified in a wedge diagram as a highly<br />
stretched structure pointing towards us, as can be seen<br />
in Fig. 7.2.<br />
Mass concentrations of smaller density have the opposite<br />
effect: galaxies that are closer to us than the center<br />
of this overdensity move towards the concentration,<br />
hence away from us. Therefore their redshift distance s<br />
is larger than their true distance D. Conversely, the peculiar<br />
velocity of galaxies behind the mass concentration<br />
is pointing towards us, so their s is smaller than their true<br />
distance. If we now consider galaxies that are located<br />
on a spherical shell around this mass concentration, this<br />
sphere in physical space becomes an oblate ellipsoid<br />
with symmetry axis along the line-of-sight in redshift<br />
space. This effect is illustrated in Fig. 8.6.<br />
Hence, the distortion between physical space <strong>and</strong><br />
redshift space is caused by peculiar velocities which<br />
manifest themselves in the transformation (8.7) of the<br />
radial coordinate in space (thus, the one along the lineof-sight).<br />
Due to this effect, the correlation function of<br />
galaxies is not isotropic in redshift space. The reason for<br />
this is the relation between the density field <strong>and</strong> the corresponding<br />
peculiar velocity field. Specializing (7.49)<br />
to the current epoch <strong>and</strong> using the relation (8.1) between<br />
the density fields of matter <strong>and</strong> of galaxies, we obtain<br />
u(x) = β H ∫<br />
0<br />
4π<br />
d 3 y δ g ( y)<br />
where we defined the parameter<br />
β := Ω0.6 m<br />
b<br />
y − x<br />
|y − x| 3 , (8.8)<br />
. (8.9)<br />
This relation between the density field of galaxies <strong>and</strong><br />
the peculiar velocity is valid in the framework of linear<br />
perturbation theory under the assumption of linear<br />
biasing. The anisotropy of the correlation function is<br />
now caused by this correlation between u(x) <strong>and</strong> δ g (x),<br />
<strong>and</strong> the degree of anisotropy depends on the parameter<br />
β. Since the correlation function is anisotropic, this<br />
likewise applies to the power spectrum.<br />
Cosmological Constraints. Indeed, the anisotropy of<br />
the correlation function can be measured, as is shown in<br />
Fig. 8.7 for the 2dFGRS (where in this figure, the usual