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A gravity-driven inflation is shown to arise from a simple higher dimensional universe. In vacuum, the shear of $n>1$ contracting dimensions is able to inflate the remaining three spatial dimensions. Said another way, the expansion of the…

广义相对论与量子宇宙学 · 物理学 2009-10-22 Janna Levin

Here $f(R)$-cosmology is discussed using a different approach. This model explains early-inflation, emergence of cosmic background radiation at the exit from inflation, cosmic deceleration during radiation-dominance followed by deceleration…

广义相对论与量子宇宙学 · 物理学 2008-10-09 S. K. Srivastava

We consider the non-commutative inflation model of [3] in which it is the unconventional dispersion relation for regular radiation which drives the accelerated expansion of space. In this model, we study the evolution of linear cosmological…

高能物理 - 理论 · 物理学 2008-11-26 Seoktae Koh , Robert H. Brandenberger

Cosmic inflation provides a mechanism for generating the early density perturbations that seeded the large-scale structures we see today. Primordial non-Gaussianity is among the most promising of few observational tests of physics at this…

宇宙学与河外天体物理 · 物理学 2011-10-10 Marilena LoVerde , Simone Ferraro , Kendrick M. Smith

We give a detailed presentation of a recently proposed mechanism of generating the energy scale of inflation by loop effects in quantum cosmology. We discuss the quantum origin of the early inflationary Universe from the no-boundary and…

广义相对论与量子宇宙学 · 物理学 2011-08-17 A. O. Barvinsky , A. Yu. Kamenshchik , I. V. Mishakov

We consider the Standard Models of particle physics and hot big bang cosmology, and review the theoretical and experimental motivations for extending these models to include supersymmetry and inflation. An obvious extension would be to…

高能物理 - 唯象学 · 物理学 2008-11-26 S. F. King , D. A. J. Rayner

In the framework of scalar-tensor theories of gravity, we construct a new kind of cosmological model that conflates inflation and ekpyrosis. During a phase of conflation, the universe undergoes accelerated expansion, but with crucial…

高能物理 - 理论 · 物理学 2016-09-07 Angelika Fertig , Jean-Luc Lehners , Enno Mallwitz

Cosmic inflation provides a window to the highest energy densities accessible in nature, far beyond those achievable in any realistic terrestrial experiment. Theoretical insights into the inflationary era and its observational probes may…

A gauge singlet scalar with non-minimal coupling to gravity can drive inflation and later freeze out to become cold dark matter. We explore this idea by revisiting inflation in the singlet direction (S-inflation) and Higgs Portal Dark…

宇宙学与河外天体物理 · 物理学 2015-11-18 Felix Kahlhoefer , John McDonald

We consider General Relativity with matter and radiation, one of these fluids being coupled to vacuum. We find that Universe dynamics starts by an inflation phase if the coupled fluid has a negative energy density at early time. Then, there…

广义相对论与量子宇宙学 · 物理学 2014-04-15 Stéphane Fay

I propose a unified model of particle physic and cosmology based on both a new extension of the standard particle model and the fundamental principle of the standard cosmology. Beyond the SM, I introduce several species of dark fields with…

综合物理 · 物理学 2025-05-13 Wei-Min Yang

Future measurements of primordial non-Gaussianity can reveal cosmologically produced particles with masses of order the inflationary Hubble scale and their interactions with the inflaton, giving us crucial insights into the structure of…

高能物理 - 唯象学 · 物理学 2018-05-15 Soubhik Kumar , Raman Sundrum

A warm inflationary universe model in loop quantum cosmology is studied. In general we discuss the condition of inflation in this framework. By using a chaotic potential, $V(\phi)\propto \phi^2$, we develop a model where the dissipation…

宇宙学与河外天体物理 · 物理学 2014-11-21 Ramon Herrera

The creation of ultra-light dark particles in the late-time FLRW spacetime provides a cosmological model in accordance with precise observational tests. The matter creation backreaction implies in this context a vacuum energy density…

宇宙学与河外天体物理 · 物理学 2012-10-11 Saulo Carneiro

We construct supersymmetric unified models which automatically lead to a period of inflation. The models all involve a U(1) symmetry which does not belong to the MSSM. We consider three different types of models depending on whether this…

高能物理 - 唯象学 · 物理学 2009-10-30 R. Jeannerot

In this work, we propose a model of warm inflation driven by axion-like particles interacting with $U(1)$ gauge fields, with implications for the early universe's thermal evolution. By extending traditional warm inflation models, we…

宇宙学与河外天体物理 · 物理学 2025-07-24 Asma Alaei , Sukannya Bhattacharya , Vahid Kamali

We consider inflation in a universe with a positive cosmological constant and a nonminimally coupled scalar field, in which the field couples both quadratically and quartically to the Ricci scalar. When considered in the Einstein frame and…

广义相对论与量子宇宙学 · 物理学 2015-08-21 Dražen Glavan , Anja Marunović , Tomislav Prokopec

In this paper, we study the cosmological inflation phenomenon in symmergent gravity theory. Symmergent gravity is a novel framework which merges gravity and the standard model (SM) so that the gravity emerges from the matter loops and…

宇宙学与河外天体物理 · 物理学 2024-03-04 Nilay Bostan , Canan Karahan , Ozan Sargın

If cosmic inflation was driven by an electrically neutral scalar field stable on cosmological time scales, the field necessarily constitutes all or part of dark matter (DM). We study this possibility in a scenario where the inflaton field…

高能物理 - 唯象学 · 物理学 2019-03-13 Juan P. Beltrán Almeida , Nicolás Bernal , Javier Rubio , Tommi Tenkanen

It is widely accepted that the primordial universe experienced a brief period of accelerated expansion called inflation. This scenario provides a plausible solution to the horizon and flatness problems. However, the particle physics…

广义相对论与量子宇宙学 · 物理学 2020-07-17 Sebastien Galtier , Jason Laurie , Sergey V. Nazarenko
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