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on
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Outline
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INFLATION: WHY SO IMPORTANT?
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What is inflation?
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The rise and fall ... of the comoving Hubble horizon
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INFLATION:
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When? Fitting into the Big Picture
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Initial conditions
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HOW? INFLATION and THE INFLATON
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Observational predictions
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Zoology of inflationary models
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Inflation dynamics and the level of gravity waves
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Classifying inflationary models
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Non-canonical kinetic term
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......and multi-field models of inflation
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......and vector fields during inflation?
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Models with primordial vector fields during inflation
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The f F2 model: power spectrum and bispectrum
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Main message about IR modes:
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Effective Field Theory approach to inflation and new symmetry breaking patterns
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The Action up to third-order from the EFT expansion
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Condensed Matter Cosmology??
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Current observational status
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Why Inflation is sensitive to high-energy fundamental physics?
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We have a dream........
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Why gravity waves of inflation are important?
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Primordial non-Gaussianity
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Why primordial NG is important?
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A reminder......
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Another good reason: Maldacena consistency relations
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Shapes of NG: local NG
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Equilateral NG
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LESSON: NG...IT'S NOT JUST A NUMBER
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Observational limits set by Planck
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Implications for inflation models
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Planck limits on trispectra
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What can we expect in the future? Crossing critical thresholds
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Oscillatory features
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The nature of gravitational waves I
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The nature of gravitational waves I These observables can be signatures of new physics.
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Present constraints on tensor NG hkihk2hk3
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Determining the nature of Gravitational Waves II
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Measuring the Energy Scale of Inflation with Large Scale Structures
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Other example
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Chirality in the vybispectrum
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Chiral GWs: detection prospects via CMB bispectra
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Chiral scalar-tensor models: theoretical predictions
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New avenues: Anisotropies of SGWB from inflation and primordial non-Gaussianity**
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The heritage of inflation
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Conclusions: looking into the future
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The fd F2 model: power spectrum and bispectrum
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The 12b F2 model: some highlights
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Search in Presentation
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New future/futuristic observational strategies for PNG
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Expected constraints with SPHEREx
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Open questions
Description:
Explore the inflationary paradigm in cosmology through this comprehensive lecture from the Physics of the Early Universe online program. Delve into the importance of inflation, its role in the Big Bang theory, and how it addresses initial condition problems. Examine various inflationary models, including multi-field and vector field models, and their observational predictions. Investigate primordial non-Gaussianity, its significance, and current observational limits. Learn about gravitational waves from inflation and their potential for probing high-energy physics. Discuss new avenues in cosmological research, including anisotropies in the stochastic gravitational wave background. Conclude with an overview of future observational strategies and open questions in the field of cosmic inflation.

The Inflationary Paradigm by Nicola Bartolo

International Centre for Theoretical Sciences
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