Red Tilt in CMB | Explaining Inflation & Measurement

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SUMMARY

The discussion centers on the concept of 'red tilt' in cosmology, which refers to the shape of the spectrum of density perturbations. Specifically, a red tilt occurs when the primordial power spectrum follows the relation P(k) ∝ k^(n - 1) with n < 1, indicating greater power on large scales. This phenomenon is observed in the Cosmic Microwave Background (CMB), where a red spectrum results in larger anisotropies at low CMB multipoles. While inflationary models like chaotic and 'new' inflation predominantly predict red spectra, alternative models such as hybrid inflation can yield blue spectra.

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  • Understanding of primordial density perturbations
  • Familiarity with the Cosmic Microwave Background (CMB)
  • Knowledge of power spectrum analysis in cosmology
  • Basic grasp of inflationary models in cosmology
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  • Research the implications of primordial density perturbations on CMB measurements
  • Study the differences between red and blue tilted spectra in cosmological models
  • Explore chaotic and 'new' inflation models in detail
  • Investigate hybrid inflation and its predictions regarding power spectra
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Astronomers, cosmologists, and students of theoretical physics interested in understanding the implications of inflation on the structure of the universe and the analysis of the Cosmic Microwave Background.

skydivephil
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Can anyone give a good explnanation of red tilt in comsology? why inflation predicts this and how its measured in the CMb? Many thanks.
 
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A 'red tilt' refers to the shape of the spectrum of density perturbations. The primordial density perturbations are what give rise to the temperature anisotropies measured in the CMB. We can therefore use the CMB to constrain this spectrum. A simple ansatz for the shape of the primordial power spectrum is

P(k) \propto k^{n - 1}

where k is the wavenumber of the perturbation (this power spectrum is the Fourier transform of the spatial correlation function, and so small k corresponds to large-scale perturbations.) For n &lt; 1, one sees that there is more power on large scales -- in the infrared. This is called a red spectrum, or a 'red tilt'. Conversely, if n &gt; 1, there is more power on small scales and the spectrum is said to be blue tilted. In the CMB, a red spectrum would indicate itself by giving larger anisotropy on large scales (low CMB multipoles).

Inflation does not exclusively predict a red spectrum -- it can predict both blue and red. It just so happens that the more popular models, like chaotic and 'new' inflation, predict red spectra. However, simple models of hybrid inflation give blue spectra, for example.
 

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