Primordial Non‐Gaussianities from Inflation Models
Первичные негауссовости в моделях инфляции
2010-01-01
SCID: 54.1/rbtn2f3e
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early-universe cosmologyinflation modelsinflationary dynamicsnon-Gaussian profilesprimordial non-Gaussianities
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Abstract (AI)
This is a pedagogical review on primordial non‐Gaussianities from inflation models. We introduce formalisms and techniques that are used to compute such quantities. We review different mechanisms which can generate observable large non‐Gaussianities during inflation, and distinctive signatures they leave on the non‐Gaussian profiles. They are potentially powerful probes to the dynamics of inflation. We also provide a nontechnical and qualitative summary of the main results and underlying physics.
Key Findings
1
Different inflationary mechanisms generate distinctive non-Gaussian profiles that can probe inflationary dynamics.
2
It introduces formalisms and computational techniques for calculating primordial non-Gaussianity observables.
3
It surveys mechanisms capable of producing observable large non-Gaussianities during inflation.
4
The paper provides a pedagogical review of primordial non-Gaussianities generated by inflationary models.
5
The review includes a qualitative, nontechnical summary of the main results and underlying physical mechanisms.
Research Object
primordial non-Gaussianities generated during inflation
Research Subject
mechanisms generating observable large non-Gaussianities and their distinctive non-Gaussian profiles as probes of inflationary dynamics
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Publication Date
2010-01-01
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