I Fourier transform of the density fluctuation

Click For Summary
The discussion centers on the Fourier transform of density fluctuations in cosmology, specifically the equation governing the evolution of these fluctuations. The equation presented is a second-order differential equation that describes the dynamics of the density fluctuation, δ, in terms of the scale factor H and matter density Ω_m. The Fourier transform of the density fluctuation is defined, leading to a similar differential equation for δ_k, the Fourier-transformed fluctuation. The participants express confusion about the solution to this equation, suggesting that a Gaussian function may be the only viable solution. The textbook referenced is "Introduction to Cosmology" by Barbara Ryden, which provides the relevant equations and context.
happyparticle
Messages
490
Reaction score
24
TL;DR
Computing the Fourier transform of the density fluctuation.
There is a Fourier transform that I don't really understand in my textbook.

I have the following equation:
##\ddot{\delta} + 2H\dot{\delta} -\frac{3}{2} \Omega_m H^2 \delta = 0##

Then using the Fourier transform:
##\delta_{\vec{k}} = \frac{1}{V} \int \delta(\vec{r}) e^{i \vec{k} \cdot \vec{r}} d^3 r##

Where ##\delta(\vec{r})## is the density fluctuation.

We get
##\ddot{\delta_{\vec{k}}} + 2H\dot{\delta_{\vec{k}}} -\frac{3}{2} \Omega_m H^2 \delta_{\vec{k}} = 0##


The only function that does that is a gaussian function, I guess. I don't understand the process here.

Thank you
 
Space news on Phys.org
PeterDonis said:
Which textbook?
Introduction to Cosmology second edition by Barbara Ryden (p.215-219)
 

Similar threads

  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 12 ·
Replies
12
Views
2K
  • · Replies 9 ·
Replies
9
Views
1K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 7 ·
Replies
7
Views
2K