Avi Nandi
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Can anyone give an idea about primordial non gaussianity in a popular way??
Primordial non-Gaussianity refers to the non-Gaussian distribution observed in the temperature anisotropy of the cosmic microwave background (CMB). This phenomenon is discussed in detail in the paper "Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence" (https://arxiv.org/abs/0712.1148). The statistical properties of temperature variations in the CMB can deviate from Gaussianity, leading to correlated amplitudes and distributions with fatter tails. Current models predict no evidence of such deviations, as confirmed by the study "https://arxiv.org/abs/1502.01592".
PREREQUISITESAstronomers, cosmologists, and researchers in theoretical physics who are interested in the statistical properties of the cosmic microwave background and the implications of inflationary models on cosmic structure formation.
The super short version is that it's all about the statistical properties of the temperature variations in the CMB.Avi Nandi said:Can anyone give an idea about primordial non gaussianity in a popular way??