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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

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