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We consider a novel model of cosmic inflation. In our model one does not need any specific matter field to drive inflation, but inflation stems from the microscopic, Planck scale structure of spacetime, thus being of quantum gravitational…

广义相对论与量子宇宙学 · 物理学 2014-08-28 Jarmo Mäkelä

In the framework of superstring compactifications with N=1 supersymmetry spontaneously broken, (by either geometrical fluxes, branes or else), we show the existence of new inflationary solutions. The time-trajectory of the scale factor of…

高能物理 - 理论 · 物理学 2008-11-26 Costas Kounnas , Herve Partouche

Recent observations of large-scale statistical isotropy violations have prompted the adoption of anisotropic cosmological models that account for inherent directional curvature. Studies of these anisotropic spacetimes have shown how they…

广义相对论与量子宇宙学 · 物理学 2026-05-22 Devika J. S. , Tanay Gupta , Sukanta Panda

In a previous paper, two of the authors presented a "regulated" picture of eternal inflation. This picture both suggested and drew support from a conjectured discontinuity in the amplitude for tunneling from positive to negative vacuum…

高能物理 - 理论 · 物理学 2009-11-11 A. Aguirre , T. Banks , M. Johnson

This paper discusses the problem of inflation in the context of Friedmann-Robertson-Walker Cosmology. We show how, after a simple change of variables, one can quantize the problem in a way which parallels the classical discussion. The…

高能物理 - 理论 · 物理学 2007-05-23 Marvin Weinstein , Ratin Akhoury

A new model of nonlinear electrodynamics with dimensional parameters $\beta$ and $\gamma$ is proposed. The principles of causality and unitarity are studied. We show that a singularity of the electric field at the origin of charges is…

广义相对论与量子宇宙学 · 物理学 2020-04-29 S. I. Kruglov

By demanding the validity of an effective field theory description during inflation, in this note we derive some peculiar inequalities among the three interesting stringy and cosmological parameters, namely the tensor-to-scalar ratio ($r$),…

高能物理 - 理论 · 物理学 2016-07-04 Anupam Mazumdar , Pramod Shukla

In the standard picture, the inflationary universe is in a supercooled state which ends with a short time, large scale reheating period, after which the universe goes into a radiation dominated stage. An alternative is proposed here in…

高能物理 - 唯象学 · 物理学 2009-10-30 Arjun Berera

We examine inflationary models in the $f(R, T)$ gravity framework where we have a conformal constant and an $RT$-mixing term apart from an R term. The RT-mixing term introduces non-minimal coupling between gravity and matter. We consider…

广义相对论与量子宇宙学 · 物理学 2025-04-16 Sohan Kumar Jha , Anisur Rahaman

We consider the compactification of (d+n)-dimensional pure gravity and of superstring/M-theory on an n-dimensional internal space to a d-dimensional FLRW cosmology, with spatial curvature k=-1,0,+1, in Einstein conformal frame. The internal…

高能物理 - 理论 · 物理学 2009-11-10 Mattias N. R. Wohlfarth

We investigate the inflationary expansion of the universe induced by higher curvature corrections in M-theory. The inflationary evolution of the geometry is discussed in ref.[1], thus we succeed to analyse metric perturbations around the…

高能物理 - 理论 · 物理学 2020-09-15 Kazuho Hiraga , Yoshifumi Hyakutake

In this paper, we explore the equivalence between two theories, namely f(R) and scalar-tensor theories of gravity. We use this equivalence to explore several f(R) toy models focusing on the inflation epoch of the early universe. The study…

广义相对论与量子宇宙学 · 物理学 2018-11-21 Joseph Ntahompagaze , Jean Damascene Mbarubukeye , Shambel Sahlu , Amare Abebe

A novel scalar field free approach to cosmic inflation is presented. The inflationary Universe and the radiation dominated Universe are shown, within the framework of unified brane cosmology, to be two different phases governed by one and…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Aharon Davidson , Ilya Gurwich

From a model-building perspective, the inflationary sector might very well have no direct couplings to other species, apart from inevitable gravitational interactions. Within the context of General Relativity, a thermal universe can still…

宇宙学与河外天体物理 · 物理学 2019-11-11 Daniel G. Figueroa , Erwin H. Tanin

We show that the constraints which follow from the {\it Trans-Planckian Censorship Conjecture} for inflationary cosmology can be strengthened if the pre-inflationary universe was dominated by radiation. The resulting upper bound on the…

高能物理 - 理论 · 物理学 2020-04-01 Robert Brandenberger , Edward Wilson-Ewing

The recent measurements of cosmological parameters by the Planck collaboration favors inflationary models with a redshifted spectrum and a very low tensor-to-scalar ratio. Two well-studied scenarios in the particle physics/string theory…

高能物理 - 唯象学 · 物理学 2014-01-31 Sean Downes

We describe a scenario for inflation in the framework of non-critical string theory, which does not employ an inflaton field. There is an exponential expansion of the volume of the Universe, induced by enormous entropy production in the…

高能物理 - 理论 · 物理学 2009-09-11 J. Ellis , N. E. Mavromatos , D. V. Nanopoulos

We study a scalar-tensor cosmological model where the Einstein tensor is non-minimally coupled to the free scalar field dynamics. Using FRW metric, we investigate the behavior of scale factor for vacuum, matter and dark energy dominated…

广义相对论与量子宇宙学 · 物理学 2015-08-06 F. Darabi , A. Parsiya

We study the evolution of simple cosmic string loop solutions in an inflationary universe. We show, for the particular case of circular loops, that periodic solutions do exist in a de Sitter universe, below a critical loop radius $R_c…

高能物理 - 唯象学 · 物理学 2008-11-26 P. P. Avelino , C. J. A. P. Martins , E. P. S. Shellard

The early universe according to the big bang and the grand unified theories is discussed. The shortcomings of big bang are summarized together with their resolution by inflationary cosmology. Inflation, the subsequent oscillation and decay…

高能物理 - 唯象学 · 物理学 2007-05-23 George Lazarides