Why is the Primordial Power Spectrum Defined as P(k) = (k^3)/(2π^2)|w_k|^2?

In summary, the power spectrum is defined as the Fourier transform of the correlation function of density perturbations, represented by the equation P(k) = (k^3)/(2π^2) * |w_k|^2, where w_k is the mode function. This definition helps to understand how different frequencies contribute to the spatial density perturbation, as indicated by the constant C in the equation. However, the exact reason for defining the power spectrum in this way is not stated in cosmology books and papers.
  • #1
shinobi20
267
19
Why is the power spectrum defined as
##P(k) = \frac{k^3}{2π^2} |w_k|^2 ##
where ##w_k## is the mode function?

Cosmology books and papers just states that it is defined that way but there are no details on why.
 
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  • #2
The power spectrum is defined as the Fourier transform of the correlation function of density perturbations. Does this help? Can you write down the expression of the correlation function of density (of curvature) perturbations?
 
  • #3
bapowell said:
The power spectrum is defined as the Fourier transform of the correlation function of density perturbations. Does this help? Can you write down the expression of the correlation function of density (of curvature) perturbations?
Let ##ξ(r)## be the two point correlation function, then as you said, we define (why?) the power spectrum as

##P(k) = C∫ ξ(r) e^{-ikx} d^3r##

where C is a constant
 
  • #4
Because the power spectrum tells you how the various frequencies contribute to the spatial density perturbation. That's generally what the Fourier transform tells you.
 

1. What is the Primordial Power Spectrum?

The Primordial Power Spectrum is a measure of the distribution of energy in the early universe. It shows the relative strength of fluctuations in the density of matter at different length scales just after the Big Bang.

2. How is the Primordial Power Spectrum measured?

The Primordial Power Spectrum is typically measured using data from cosmic microwave background (CMB) radiation observations. This radiation is an imprint of the universe just 380,000 years after the Big Bang and contains valuable information about the early universe.

3. What does the Primordial Power Spectrum tell us about the early universe?

The Primordial Power Spectrum provides valuable information about the initial conditions of the universe, such as the density and distribution of matter. It also helps scientists understand the processes that drove the evolution of the universe from its infancy to its current state.

4. How does the Primordial Power Spectrum influence the formation of structures in the universe?

The Primordial Power Spectrum plays a crucial role in the formation of large-scale structures such as galaxies and clusters of galaxies. It determines the initial density fluctuations that eventually lead to the formation of these structures through the process of gravitational collapse.

5. Are there different theories about the shape of the Primordial Power Spectrum?

Yes, there are different theories about the shape of the Primordial Power Spectrum, and scientists are continually refining and testing these theories with new observations and data. Some of the most well-known theories include the inflationary model, which predicts a nearly flat spectrum, and the scale-invariant spectrum, which predicts a power law relationship between the density fluctuations and length scales.

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