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Main Author: Dimopoulos, Konstantinos
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2402.19086
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author Dimopoulos, Konstantinos
author_facet Dimopoulos, Konstantinos
contents We briefly discuss cosmic inflation, which is the dominant paradigm for the generation of the large scale structure in the Universe and also for arranging for the initial conditions of the hot Big Bang. We then present quintessential inflation, which also accounts of the observed dark energy. We discuss how quintessential inflation can be successfully modelled in modified gravity in the Palatini formalism. Finally, we focus on the generation of primordial gravitational waves by inflation and how their spectrum can be enhanced when the early Universe goes through periods of stiff equation of state. This results in gravitational waves with a characteristic spectrum, which may well be observed in the near future, providing insights for the background theory.
format Preprint
id arxiv_https___arxiv_org_abs_2402_19086
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Cosmic Inflation, Dark Energy and Gravitational Waves
Dimopoulos, Konstantinos
High Energy Physics - Phenomenology
We briefly discuss cosmic inflation, which is the dominant paradigm for the generation of the large scale structure in the Universe and also for arranging for the initial conditions of the hot Big Bang. We then present quintessential inflation, which also accounts of the observed dark energy. We discuss how quintessential inflation can be successfully modelled in modified gravity in the Palatini formalism. Finally, we focus on the generation of primordial gravitational waves by inflation and how their spectrum can be enhanced when the early Universe goes through periods of stiff equation of state. This results in gravitational waves with a characteristic spectrum, which may well be observed in the near future, providing insights for the background theory.
title Cosmic Inflation, Dark Energy and Gravitational Waves
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2402.19086