![]() | ![]() |
Astron. Astrophys. 326, 433-441 (1997) 3. Correlation functionsThe mathematical tools that allow important filtered information to be extracted from the distribution of particles are the correlation functions. These will enable us to ascertain whether the distribution is Poissonian, or how large the difference is with respect to a Poissonian distribution. Hereafter, I define certain functions that contain the symbol
(i) In this case, the average is calculated according to the expression where
(ii) In this case, the average calculation is conducted by means of the expression where
The definitions that follow include an expansion with the second averaging method. 3.1. Particle-particle two-point correlation functionThe density of the particles is
The two-point correlation function for particles without
autocorrelation (
In order to simplify the notation, the mass dependence of U will not be indicated in what follows. A straightforward calculation shows that If we assume isotropy, the function only depends on
3.2. Mass-mass two-point correlation functionThe mass density is
With isotropy, the function depends on
3.3. Mass-particle two-point correlation functionWith the same philosophy in mind, we define other functions as the two-point correlation function mass-particle: With isotropy, the function depends on
3.4. Mass-mass-particle three-point correlation functionThis function is defined as follows: With isotropy, this function depends on three variables:
![]() ![]() ![]() ![]() © European Southern Observatory (ESO) 1997 Online publication: October 15, 1997 |