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相关论文: Special cases of the Multi-Measure Model -- unders…

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The multi-measures model applied to cosmology has been recently shown to reproduce qualitatively the expected stages of the Universe evolution, along with some unexpected features. In this article, we continue its exploration with a…

广义相对论与量子宇宙学 · 物理学 2019-03-04 Denitsa Staicova

We consider the scale-invariant inflationary model studied in [1]. The Lagrangian includes all the scale-invariant operators that can be built with combinations of $R$, $R^2$ and one scalar field. The equations of motion show that the…

广义相对论与量子宇宙学 · 物理学 2017-03-14 Giovanni Tambalo , Massimiliano Rinaldi

Two models that unify warm inflation with dark matter and dark energy are proposed. In the models, a single scalar field is responsible for the early expansion of the universe through the process of dissipative warm inflation and then acts…

广义相对论与量子宇宙学 · 物理学 2021-11-30 Xiao-Min Zhang , Kai Li , Yi-Fu Guo , Peng-Cheng Chu. He Liu , Jian-Yang Zhu

A two scalar field model that incorporates non Riemannian Measures of integration or usually called Two Measures Theory (TMT) is introduced, in order to unify the early and present universe. In the Einstein frame a K-essence is generated…

广义相对论与量子宇宙学 · 物理学 2023-12-08 Eduardo Guendelman , Ramon Herrera

We consider the cosmological application of a (variant of) relatively newly proposed model \cite{1609.06915} unifying inflation, dark energy, dark matter, and the Higgs mechanism. The model was originally defined using additional…

广义相对论与量子宇宙学 · 物理学 2019-06-21 Denitsa Staicova , Michail Stoilov

We describe a new type of gravity-matter models where gravity couples in a non-conventional way to two distinct scalar fields providing a unified Lagrangian action principle description of: (a) the evolution of both "early" and "late"…

广义相对论与量子宇宙学 · 物理学 2017-07-25 Eduardo Guendelman , Emil Nissimov , Svetlana Pacheva

We investigate for viable models of inflation that can successfully produce dark matter (DM) from inflaton decay process, satisfying all the constraints from Cosmic Microwave Background (CMB) and from some other observations. In particular,…

高能物理 - 唯象学 · 物理学 2022-10-19 Anish Ghoshal , Gaetano Lambiase , Supratik Pal , Arnab Paul , Shiladitya Porey

A unified multi scalar field model with three flat regions is discussed. The three flat regions are the inflation, early and late dark energy epochs. The potential is obtained by a spontaneous breaking of scale invariance generated by Non…

广义相对论与量子宇宙学 · 物理学 2022-06-22 Eduardo Guendelman , Ramon Herrera , David Benisty

We study the linear perturbations of multi-field inflationary models governed by a Lagrangian which is a general function of the scalar fields and of a global kinetic term combining their spacetime gradients with an arbitrary field space…

高能物理 - 理论 · 物理学 2008-11-26 David Langlois , Sébastien Renaux-Petel

Starting from pure multidimensional gravity with curvature-nonlinear terms but no matter fields in the initial action, we obtain a cosmological model with two effective scalar fields related to the size of two extra factor spaces. The model…

广义相对论与量子宇宙学 · 物理学 2010-04-21 K. A. Bronnikov , S. G. Rubin , I. V. Svadkovsky

In a recent work, we demonstrated that a modified gravity model in which a scalar "darkon" field is coupled to both the standard Riemannian metric and to another non-Riemannian volume form is compatible with observational data from…

广义相对论与量子宇宙学 · 物理学 2019-11-12 Denitsa Staicova , Michail Stoilov

A scenario with two subsequent periods of inflationary expansion in the very early universe is examined. The model is based on a potential motivated by symmetries being found in field theory at high energy. For various parameter sets of the…

宇宙学与河外天体物理 · 物理学 2016-01-13 Simon Schettler , Jurgen Schaffner-Bielich

A model of a universe without big bang singularity is presented, which displaysanearly inflationary period ending just before a phase transition to a deflationary epoch. The model produces enough heavy particles so as to reheat the universe…

广义相对论与量子宇宙学 · 物理学 2016-09-05 Jaume de Haro , Emilio Elizalde

We consider the history of the universe from a possible big bang or a bounce into a late period of a unified interacting dark energy - dark matter model. The model is based on the Two Measures Theories (T.M.T.) which introduces a metric…

广义相对论与量子宇宙学 · 物理学 2018-07-30 David Benisty , Eduardo I. Guendelman

The existence of the inflationary era in the early Universe seems to be strongly supported by recent CMB observations. However, only a few realistic inflation scenarios which have close relation to particle physics seem to have been known…

高能物理 - 唯象学 · 物理学 2015-01-05 Romy H. S. Budhi , Shoichi Kashiwase , Daijiro Suematsu

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

In this work, we investigate the physical aspects of the inflection-point inflation scenario and assess its observational viability in light of current Cosmic Microwave Background (CMB) data. The model we consider encapsulates the inflaton…

宇宙学与河外天体物理 · 物理学 2024-06-25 Jamerson G. Rodrigues , Vinícius Oliveira , Rodrigo von Marttens , Carlos A. de S. Pires , Jailson Alcaniz

Predictions of inflationary schemes can be influenced by the presence of extra dimensions. This could be of particular relevance for the spectrum of gravitational waves in models where the extra dimensions provide a brane-world solution to…

高能物理 - 唯象学 · 物理学 2018-03-09 Sang Hui Im , Hans Peter Nilles , Andreas Trautner

We have investigated inflationary model constructed from minimally modified gravity (MMG) theories. The MMG theory in the form of $f({\bf H}) \propto {\bf H}^{1+p}$ gravity where, ${\bf H}$ is the Hamiltonian constraint in the Einstein…

宇宙学与河外天体物理 · 物理学 2021-07-14 Jakkrit Sangtawee , Khamphee Karwan

We discuss a minimal extension of the Standard Model (SM) where a single real scalar field serves as both inflaton and dark matter. The corresponding Lagrangian contains the renormalizable interactions of the inflaton field. Quantum effects…

高能物理 - 唯象学 · 物理学 2022-05-30 Jong-Hyun Yoon
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