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相关论文: Anisotropic Kantowski-Sachs Universe from Gravitat…

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We construct general anisotropic cosmological scenarios governed by an $f(R)$ gravitational sector. Focusing then on Kantowski-Sachs geometries in the case of $R^n$-gravity, and modelling the matter content as a perfect fluid, we perform a…

广义相对论与量子宇宙学 · 物理学 2011-08-19 Genly Leon , Emmanuel N. Saridakis

We study the GMGHS spacetimes to analyze the evolution of the anisotropy universe, which can be treated as a doubly warped products manifold possessing warping functions (or scale factor) having the Kantowski-Sachs solution which represents…

广义相对论与量子宇宙学 · 物理学 2016-01-12 Jaedong Choi

It seems generic to have vacua with lower dimensionality than ours. We consider the possibility that the observable universe originated in a transition from one of these vacua. Such a universe has anisotropic spatial curvature. This may be…

高能物理 - 理论 · 物理学 2010-09-29 Peter W. Graham , Roni Harnik , Surjeet Rajendran

In the standard cosmological model, the temperature anisotropy of the cosmic microwave background is interpreted as variation in the gravitational potential at the point of emission, due to the emitter being embedded in a region ${\cal C}$…

天体物理学 · 物理学 2007-05-23 Richard Lieu

We consider a universe formed in a black hole in the Einstein--Cartan theory of gravity. The interior of a Schwarzschild black hole can be represented by the Kantowski--Sachs metric that describes a closed anisotropic universe. We use this…

广义相对论与量子宇宙学 · 物理学 2021-02-19 Nikodem Popławski

A recent paper (Martinez--Gonzalez & Sanz 1995) showed that if the universe is homogeneous but anisotropic, then the small quadrupole anisotropy in the cosmic microwave background radiation implies that the spacetime anisotropy is very…

天体物理学 · 物理学 2007-05-23 Roy Maartens , George Ellis , William Stoeger

This article describes the theory of cosmological perturbations around a homogeneous and anisotropic universe of the Bianchi I type. Starting from a general parameterisation of the perturbed spacetime a la Bardeen, a complete set of gauge…

天体物理学 · 物理学 2008-11-26 Thiago S. Pereira , Cyril Pitrou , Jean-Philippe Uzan

We investigate cosmologies where the accelerated expansion of the Universe is driven by a field with an anisotropic equation of state. We model such scenarios within the Bianchi I framework, introducing two skewness parameters to quantify…

天体物理学 · 物理学 2009-06-23 Tomi Koivisto , David F. Mota

The cosmological principle asserts that on sufficiently large scales the Universe is homogeneous and isotropic on spatial slices. To deviate from this principle requires a departure from the FLRW ansatz. In this paper we analyze the…

宇宙学与河外天体物理 · 物理学 2023-11-23 Andrei Constantin , Thomas R. Harvey , Sebastian von Hausegger , Andre Lukas

We use a path-integral approach to study the tunneling wave function in quantum cosmology with spatial topology $S^{1}\times S^{2}$ and positive cosmological constant (the Kantowski-Sachs model). If the initial scale factors of both $S^1$…

广义相对论与量子宇宙学 · 物理学 2022-09-07 Georgios Fanaras , Alexander Vilenkin

Working toward a model independent understanding of cosmic microwave background (CMB) anisotropies and their significance, we undertake a comprehensive and self-contained study of scalar perturbation theory. Initial conditions, evolution,…

天体物理学 · 物理学 2009-09-25 Wayne Hu , Naoshi Sugiyama

We show that the difference between the theoretically expected and measured by WMAP amplitude of the quadrupole fluctuations of CMB can be related to the impact of the anisotropic curvature of the homogeneous universe dominated by the dark…

天体物理学 · 物理学 2008-11-26 M. Demiański , A. G. Doroshkevich

We analyze the state space of a Bianchi-I universe with anisotropic sources. Here we consider an extended state space which includes null geodesics in this background. The evolution equations for all the state observables are derived.…

广义相对论与量子宇宙学 · 物理学 2016-02-09 Pavan K. Aluri , Sukanta Panda , Manabendra Sharma , Snigdha Thakur

A cosmological model with anisotropic dark energy is analyzed. The amount of deviation from isotropy of the equation of state of dark energy, the skewness \delta, generates an anisotropization of the large-scale geometry of the Universe,…

宇宙学与河外天体物理 · 物理学 2011-06-28 L. Campanelli , P. Cea , G. L. Fogli , L. Tedesco

The study of anisotropies in the Cosmic Microwave Background radiation is progressing at a phenomenal rate, both experimentally and theoretically. These anisotropies can teach us an enormous amount about the way that fluctuations were…

天体物理学 · 物理学 2008-11-26 Douglas Scott , Martin White

Our universe may have formed via bubble nucleation in an eternally-inflating background. Furthermore, the background may have a compact dimension--the modulus of which tunnels out of a metastable minimum during bubble nucleation--which…

高能物理 - 理论 · 物理学 2014-11-20 Jose J. Blanco-Pillado , Michael P. Salem

The detection of a time variation of the angle between two distant sources would reveal an anisotropic expansion of the Universe. We study this effect of "cosmic parallax" within the "ellipsoidal universe" model, namely a particular…

宇宙学与河外天体物理 · 物理学 2011-06-29 L. Campanelli , P. Cea , G. L. Fogli , L. Tedesco

The recent high-quality measurements of the Cosmic Microwave Background anisotropies have presented cosmologists with the possibility of studying the large scale properties of our universe with unprecedented precision. Here I review the…

高能物理 - 唯象学 · 物理学 2007-05-23 Alessandro Melchiorri

If one is willing to give up the cherished hypothesis of spatial isotropy, many interesting cosmological models can be developed beyond the simple anisotropically expanding scenarios. One interesting possibility is presented by shear-free…

宇宙学与河外天体物理 · 物理学 2015-07-22 Thiago S. Pereira , Guillermo A. Mena Marugán , Saulo Carneiro

Large-scale cosmic microwave background anisotropies in homogeneous, globally anisotropic cosmologies are investigated. We perform a statistical analysis in which the four-year data from the Cosmic Background Explorer satellite is searched…

天体物理学 · 物理学 2008-11-26 Emory. F. Bunn , Pedro Ferreira , Joseph Silk
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