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# Title: Particle Physics Models of Inflation and the Cosmological Density Perturbation

Authors: David H. Lyth (Lancaster), Antonio Riotto (CERN/Oxford)
Abstract: This is a review of particle-theory models of inflation, and of their predictions for the primordial density perturbation that is thought to be the origin of structure in the Universe. It contains mini-reviews of the relevant observational cosmology, of elementary field theory and of supersymmetry, that may be of interest in their own right. The spectral index $n(k)$, specifying the scale-dependence of the spectrum of the curvature perturbation, will be a powerful discriminator between models, when it is measured by Planck with accuracy $\Delta n\sim 0.01$. The usual formula for $n$ is derived, as well as its less familiar extension to the case of a multi-component inflaton; in both cases the key ingredient is the separate evolution of causally disconnected regions of the Universe. Primordial gravitational waves will be an even more powerful discriminator if they are observed, since most models of inflation predict that they are completely negligible. We treat in detail the new wave of models, which are firmly rooted in modern particle theory and have supersymmetry as a crucial ingredient. The review is addressed to both astrophysicists and particle physicists, and each section is fairly homogeneous regarding the assumed background knowledge.
 Comments: 156 pages, after final proof corrections and additions Subjects: High Energy Physics - Phenomenology (hep-ph); Astrophysics (astro-ph); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Theory (hep-th) Journal reference: Phys.Rept.314:1-146,1999 DOI: 10.1016/S0370-1573(98)00128-8 Cite as: arXiv:hep-ph/9807278 (or arXiv:hep-ph/9807278v4 for this version)

## Submission history

From: [view email]
[v1] Tue, 7 Jul 1998 14:37:00 GMT (155kb)
[v2] Fri, 14 Aug 1998 17:20:30 GMT (157kb)
[v3] Mon, 26 Oct 1998 18:48:25 GMT (163kb)
[v4] Tue, 16 Mar 1999 13:17:32 GMT (161kb)