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

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SUMMARY

The power spectrum in cosmology is defined as P(k) = (k^3)/(2π^2)|w_k|^2, where w_k represents the mode function. This definition arises from the Fourier transform of the two-point correlation function of density perturbations, ξ(r). The constant C in the expression P(k) = C∫ ξ(r) e^{-ikx} d^3r is crucial as it normalizes the contribution of various frequencies to the spatial density perturbation. Understanding this relationship is essential for analyzing the distribution of matter in the universe.

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  • Fourier Transform concepts
  • Two-point correlation function in cosmology
  • Density perturbations in cosmological models
  • Mode functions in quantum field theory
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  • Study the derivation of the two-point correlation function in cosmology
  • Explore the implications of the Fourier transform on density perturbations
  • Investigate the role of mode functions in quantum field theory
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shinobi20
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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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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?
 
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
 
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.
 

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