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We present a simple, exact and self-consistent cosmology with a phenomenological model of quantum creation of radiation due to decay of the scalar field. The decay drives a non-isentropic inflationary epoch, which exits smoothly to the…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Alexei Nesteruk

We present a simple and thermodynamically consistent cosmology with a phenomenological model of quantum creation of radiation due to vacuum decay. Thermodynamics and Einstein's equations lead to an equation in which $H$ is determined by the…

天体物理学 · 物理学 2008-11-26 E Gunzig , R Maartens , A Nesteruk

The present work deals with a cosmological model having particle creation mechanism in the framework of irreversible thermodynamics. In the second order non-equilibrium thermodynamical prescription, the particle creation rate is treated as…

广义相对论与量子宇宙学 · 物理学 2015-05-01 Subenoy Chakraborty , Supriya Pan , Subhajit Saha

A very simple non-singular inflationary model is presented where the unique matter content is a radiation fluid. The model slowly contracts from a very large, almost empty and flat spacetime and realizes a bounce. It is then launched to a…

广义相对论与量子宇宙学 · 物理学 2024-03-08 Piero A. P. Molinari , Paola C. M. Delgado , Rodrigo F. Pinheiro , Nelson Pinto-Neto

Perhaps the deepest mystery of our accelerating Universe in expansion is the existence of a tiny and rigid cosmological constant, $\Lambda$. Its size is many orders of magnitude below the expected one in the standard model of particle…

广义相对论与量子宇宙学 · 物理学 2015-04-03 Joan Sola , Adria Gomez-Valent

In this paper we have given a generalisation of the earlier work by Prigogine et al. who have constructed a phenomenological model of entropy production via particle creation in the very early universe generated out of the vacuum rather…

广义相对论与量子宇宙学 · 物理学 2015-06-05 G. K. Goswami , Mandwi Trivedi

On the basis of a semi-classical analysis of vacuum energy in an expanding spacetime, we describe a non-singular cosmological model in which the vacuum density decays with time, with a concomitant production of matter. During an infinitely…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Saulo Carneiro

An accelerated universe should naturally have a vacuum energy density determined by its dynamical curvature. The cosmological constant is most likely a temporary description of a dynamical variable that has been drastically evolving from…

广义相对论与量子宇宙学 · 物理学 2015-10-28 Joan Sola

In this Letter we discuss the issues of the graceful exit from inflation and of matter creation in the context of a recent scenario \cite{RHBrev} in which the back-reaction of long wavelength cosmological perturbations induces a negative…

高能物理 - 理论 · 物理学 2009-11-10 Robert Brandenberger , Anupam Mazumdar

Suppose that the early Universe starts with a quantum spacetime originated cosmological $\Lambda$-term at the Planck scale $M_{\rm pl}$. The cosmological energy density $\rho_{_{_\Lambda}}$ drives inflation and simultaneously reduces its…

广义相对论与量子宇宙学 · 物理学 2021-04-27 She-Sheng Xue

The paper deals with the mechanism of particle creation in the framework of irreversible thermodynamics. The second order non-equilibrium thermodynamical prescription of Israel and Stewart has been presented with particle creation rate,…

广义相对论与量子宇宙学 · 物理学 2016-05-04 Subenoy Chakraborty , Subhajit Saha

A nonsingular deflationary cosmology driven by adiabatic matter creation is proposed. In this scenario there is no preinflationary stage as happens in conventional inflationary models. Deflation starts from a de Sitter spacetime…

广义相对论与量子宇宙学 · 物理学 2009-10-28 J. A. S. Lima , L. R. W. Abramo

In the present model, a unified picture of cosmology from early inflation to late acceleration is obtained from $ f(R)-$ gravity with non-linear terms $ R^2 $ and $ R^5 $ of scalar curvature $R$. It is discussed that elementary particles…

广义相对论与量子宇宙学 · 物理学 2008-09-12 S. K. Srivastava

Cosmology is nowadays going through a true revolution in the quantity and quality of observations that are capable of providing crucial information about the origin and evolution of the universe. In the first years of the next millenium we…

天体物理学 · 物理学 2015-06-24 Juan Garcia-Bellido

Vacuum energy, a prediction of quantum field theory, manifests itself as a cosmological constant in general relativity. In this Letter, we propose a novel inflationary scenario driven by a bare cosmological constant $\Lambda$, which…

广义相对论与量子宇宙学 · 物理学 2026-03-25 Chengsheng Mu , Shuxun Tian , Shuo Cao , Zong-Hong Zhu

A static non-singular 10-dimensional closed Friedmann universe of Planck size, filled with a perfect fluid with an equation of state with w = -2/3, can arise spontaneously by a quantum fluctuation from nothing in 11-dimensional spacetime. A…

广义相对论与量子宇宙学 · 物理学 2009-11-11 T. R. Mongan

Current astronomical observations are successfully explained by the present cosmological paradigm based on the concordance model ($\Lambda_0$CDM + Inflation). However, such a scenario is composed of a heterogeneous mix of ingredients for…

广义相对论与量子宇宙学 · 物理学 2018-08-29 J. A. S Lima , Douglas Singleton

We investigate the creation of dark matter particles as a result of the decay of the scalar field in the framework of warm inflationary models, by using the irreversible thermodynamics of open systems with matter creation/annihilation. We…

广义相对论与量子宇宙学 · 物理学 2023-03-07 Teodora Matei , Tiberiu Harko , Gabriela Mocanu

The cosmological constant $\Lambda$ is a measure of the energy density of the vacuum. Therefore properties of the energy of the system in the metastable vacuum state reflect properties of $\Lambda = \Lambda(t)$. We analyze properties of the…

广义相对论与量子宇宙学 · 物理学 2022-03-23 Krzysztof Urbanowski

We propose a mechanism for generating an inflationary phase in the early universe without resorting to any type of scalar field(s). Instead, this accelerated expansion is driven by a dynamical "cosmological constant" in the framework of…

广义相对论与量子宇宙学 · 物理学 2022-03-18 Gabriel Leon
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