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Inflationary Cosmology: From Theory to Observations

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arxiv 1810.09934 v3 pith:NUB4NT45 submitted 2018-10-10 astro-ph.CO hep-th

J. Alberto Vazquez , Luis E. Padilla , Tonatiuh Matos This is my paper
classification astro-ph.COhep-th
keywords inflationarycosmologycurrentfieldmodelobservationsscalarsingle
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abstract

The main aim of this paper is to provide a qualitative introduction to the cosmic inflation and its relationship with current cosmological observations. The inflationary model solves many of the fundamental problems that challenge the Standard Big Bang cosmology i.e. Flatness, Horizon and Monopole problem, and additionally provides an explanation for the initial conditions observed throughout the Large-Scale Structure of the Universe, such as galaxies. In this review we describe the general solutions carry out by a single scalar field. Then with the use of current surveys, we show the constraints imposed on the inflationary parameters $(n_{\rm s},r)$ which allow us to make the connection between theoretical and observational cosmology. In this way, with the latest results, it is possible to choose or at least to constrain the right inflationary model, parameterised by a single scalar field potential $V(\phi)$.

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Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Gravitational Properties of the Monopole Bag

    hep-ph 2026-04 unverdicted novelty 6.0 of 10

    Monopole bags in axionic backgrounds gravitationally collapse into horizonless states or dyonic regular black holes that evade singularities while retaining axionic hair.

  2. Conformal symmetry, SM and Gravity

    hep-th 2026-07 conditional novelty 5.0 of 10

    A Weyl-invariant SM+mirror-dark-matter+gravity model is developed via algebraic renormalization; its conformal cohomology is claimed trivial, and the required counterterms could — the author concedes not conclusively ...

  3. Gravitational Properties of the Monopole Bag

    hep-ph 2026-04 unverdicted novelty 5.0 of 10

    Monopole bags in axion models can collapse into horizonless objects or dyonic regular black holes that evade singularities and retain axionic structure through Chern-Simons effects.

  4. Hamilton-Jacobi Approach to Inflationary Scenarios through Extended Entropies: An Observational Perspective

    astro-ph.CO 2026-05 unverdicted novelty 4.0 of 10

    Hamilton-Jacobi analysis of slow-roll inflation with non-Bekenstein-Hawking entropies yields fitted entropy parameters (δ≈1.1-1.2, α∼10^{-14}, K∼10^{-17}) consistent with ns and r data.

  5. An Analytic Formalism of Inflation for Derivative Coupled Scalar Field and Validating its predictions for Some Inflationary Potentials

    astro-ph.CO 2026-04 unverdicted novelty 4.0 of 10

    Derivative-coupled scalar field inflation produces ns and r values consistent with Planck and ACT data for power-law, alpha-attractor, arctan, hilltop, and polynomial potentials.

  6. Anomaly footprints in SM+Gravity

    hep-th 2025-10 conditional novelty 4.0 of 10

    A mirror right-handed copy of the standard model, sharing only gravity and SU(2), is claimed to be anomaly-free, proposed as dark matter, and wrapped in a Weyl-invariant early-universe solution.

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