3.3. Fractal scaling
The number of neighbors - on average - a galaxy has within a sphere of radius r is just the integral
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(4) |
When this function follows a power-law N( < r)
rD2,
the exponent is the correlation dimension, and the point pattern
is said to verify fractal scaling. There is no doubt that up to a
given scale the galaxy distribution fits rather well the fractal
picture. However, some controversy regarding the extent of the
fractal regime has motivated an interesting debate
[26,
27,
28,
7].
Nevertheless, the
new data is showing overwhelming evidence that the correlation
dimension is a scale dependent quantity. Different authors
[29,
30,
31,
32,
33,
34,
35,
36,
37]
have analyzed the more recent available redshift surveys using
N(r) or related measures with appropriate estimators. Their
results show unambiguously an increasing trend of D2
with the scale from values of D2 ~ 2 at intermediate
scales to values of D2 ~ 3 at scales larger than 30
h-1 Mpc. Moreover,
one of the strong predictions of the fractal hypothesis is that
the correlation length - the value r0 at which the
correlation function reaches the unity
(
(r0) = 1) - must increase linearly
with the depth of the sample. This seems not to be the case
[38,
39].