What is primordial non gaussianity?

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Discussion Overview

The discussion revolves around the concept of primordial non-Gaussianity, particularly in relation to the cosmic microwave background (CMB) and its temperature anisotropies. Participants explore its statistical properties, implications for inflation models, and the challenges in investigating deviations from Gaussian behavior.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants seek a popular explanation of primordial non-Gaussianity.
  • One participant describes primordial non-Gaussianity as a term for the non-Gaussian distribution detected in the CMB's temperature anisotropy.
  • Another participant explains that temperature variations in the CMB are sound waves, and deviations from Gaussianity can occur through correlated amplitudes and non-Gaussian distributions.
  • The discussion highlights that Gaussian-distributed waves can be described by the two-point correlation function, simplifying the understanding of CMB statistics.
  • Some inflation models predict significant deviations from Gaussian behavior, which could complicate investigations, although no evidence of such deviations has been found so far.

Areas of Agreement / Disagreement

Participants express varying levels of understanding and seek clarification, indicating that the concept may not be fully agreed upon or understood by all. There is no consensus on the implications or evidence regarding deviations from Gaussianity.

Contextual Notes

The discussion includes assumptions about statistical properties and the implications of Gaussian versus non-Gaussian distributions, which may not be fully resolved or universally accepted.

Avi Nandi
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Can anyone give an idea about primordial non gaussianity in a popular way??
 
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Where did you see this expression, or did you make it up?
 
Primordial non-Gaussianity is simply a term fo the non Guassian distribution detected in the temperature anisotropy of the cosmic microwave background. One of the better known discussions of this phenomenon is probably https://arxiv.org/abs/0712.1148, Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence.
 
Avi Nandi said:
Can anyone give an idea about primordial non gaussianity in a popular way??
The super short version is that it's all about the statistical properties of the temperature variations in the CMB.

Those temperature variations are sound waves, and at each frequency and direction of motion, if they are Gaussian, the amplitude of the resulting wave is drawn from an independent Gaussian distribution (also known as a Normal distribution). Deviations from this strict Gaussianity come in two ways:
1. The amplitudes of the waves can be correlated with one another.
2. The distribution of amplitudes differs from a Gaussian distribution (typically having fatter tails, meaning large deviations are more frequent than expected from a pure Gaussian).

The benefit of having Gaussian-distributed waves is that they can be perfectly-described by what is known as the two-point correlation function (which is the statistical variance between two points as a function of distance between the two points, independent of direction). This fact has a lot of really neat mathematical properties which make understanding the statistics of the CMB really easy. It means, for example, that all of the information about the temperature variation of the CMB is encoded in its power spectrum.

But what if this assumption isn't the case? Lots of more complex inflation models predict significant deviations from Gaussian behavior. These deviations can become far more challenging to investigate, just due to the more complex mathematics involved. So far, there is no evidence of deviation from Gaussianity:
https://arxiv.org/abs/1502.01592
 
Thanks Chronos and Kimbyd.
 

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