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Modern cosmology rests on the working assumption that the Universe is isotropic and homogeneous at large scales. Here, we document a number of anomalous observations pointing to an anisotropic Universe in a direction consistent with the CMB…

宇宙学与河外天体物理 · 物理学 2022-03-22 Eoin Ó Colgáin

We investigate the possibility that the matter of the universe has a significant component (the quintessence component) determined by the equation of state $p=w\rho$, with $w<0$. Here, we find conditions under which a closed model may look…

天体物理学 · 物理学 2009-10-31 Norman Cruz , Sergio del Campo , Ramon Herrera

We construct general anisotropic cosmological scenarios governed by an $f(R)=R^n$ gravitational sector. Focusing then on some specific geometries, and modelling the matter content as a perfect fluid, we perform a phase-space analysis. We…

广义相对论与量子宇宙学 · 物理学 2014-03-11 Genly Leon

We review a technique for solving a class of classical linear partial differential systems of relevance to physics in Minkowski spacetime. All the equations are amenable to analysis in terms of complex solutions in the kernel of the scalar…

广义相对论与量子宇宙学 · 物理学 2022-02-23 Robin W. Tucker , Timothy J. Walton

We expose the scenarios of primordial baryon-photon plasma evolution within the framework of the Milne-like universe models. Recently, such models find a second wind and promise an inflation-free solution of a lot of cosmological puzzles…

广义相对论与量子宇宙学 · 物理学 2019-01-09 S. L. Cherkas , V. L. Kalashnikov

An anisotropic cosmological model with a gauge field, presented by spatially homogeneous SU(2)-symmetric Yang-Mills potentials, is considered. Bianchi-I model with axial symmetry is analyzed; a new exact solution, which describes the early…

广义相对论与量子宇宙学 · 物理学 2025-05-06 Alexander B. Balakin , Gleb B. Kiselev

We study evolution of manifolds after their creation at high energies. Several kinds of gravitational Lagrangians with higher derivatives are considered. It is shown analytically and confirmed numerically that an asymptotic growth of the…

广义相对论与量子宇宙学 · 物理学 2019-12-30 Yana Lyakhova , Arkady A. Popov , Sergey G. Rubin

We confirm for the first time the existence of distinctive halo bias associated with the quadrupolar type of statistical anisotropy (SA) of the linear matter density field using cosmological $N$-body simulations. We find that the…

宇宙学与河外天体物理 · 物理学 2025-05-19 Shogo Masaki , Maresuke Shiraishi , Takahiro Nishimichi , Teppei Okumura , Shuichiro Yokoyama

We consider a spatially homogeneous and isotropic cosmological model where Dirac spinors are coupled to classical gravity. For the Dirac spinors we choose a Hartree-Fock ansatz where all one-particle wave functions are coherent and have the…

数学物理 · 物理学 2014-04-23 Felix Finster , Christian Hainzl

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 look for necessary conditions such that minimally coupled scalar-tensor theory with a massive scalar field and a perfect fluid in the Bianchi type I model isotropises. Then we derive the dynamical asymptotical properties of the Universe.

广义相对论与量子宇宙学 · 物理学 2007-05-23 Stephane Fay

In this paper, we study a projectable Ho\v{r}ava-Lifshitz cosmology without the detailed balance condition minimally coupled to a non-linear self-coupling scalar field. In the minisuperspace framework, the super Hamiltonian of the presented…

广义相对论与量子宇宙学 · 物理学 2021-02-25 Fatimah Tavakoli , Babak Vakili , Hossein Ardehali

We recently derived exact solutions for the scalar, vector and tensor mode functions of a single, minimally coupled scalar plus gravity in an arbitrary homogeneous and isotropic background. These solutions are applied to obtain improved…

天体物理学 · 物理学 2009-11-10 N. C. Tsamis , R. P. Woodard

We compute the covariance expected between the spherical harmonic coefficients $a_{\ell m}$ of the cosmic microwave temperature anisotropy if the universe had a compact topology. For fundamental cell size smaller than the distance to the…

天体物理学 · 物理学 2009-11-10 N. G. Phillips , A. Kogut

Spatially flat loitering universe models have recently been shown to arise in the context of brane world scenarios. Such models allow more time for structure formation to take place at high redshifts, easing, e.g., the tension between the…

天体物理学 · 物理学 2009-11-10 O. Elgaroy , D. F. Mota , T. Multamaki

In this article we compute the density of scalar and Dirac particles created by a cosmological anisotropic Bianchi type I universe in the presence of a time varying electric field. We show that the particle distribution becomes thermal when…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Victor M. Villalba , Walter Greiner

Cosmological solution to the gravitational field equations in the generalized Randall-Sundrum model for an anisotropic brane with Bianchi I geometry and perfect fluid as matter sources has been considered. The matter on the brane is…

广义相对论与量子宇宙学 · 物理学 2019-12-16 Rikpratik Sengupta , Prasenjit Paul , Bikash Chandra Paul , Saibal Ray

We investigate the canonical quantization in the framework of N=1 simple supergravity for the case of a very simple gravitational midisuperspace described by Gowdy $T^3$ cosmological models. We consider supersymmetric quantum cosmology in…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Alfredo Macias , Abel Camacho , Jutta Kunz , Claus Laemmerzahl

We study the effect of the non-commutativity on the creation of scalar particles from vacuum in the anisotropic universe space-time. We derive the deformed Klein-Gordon equation up to second order in the non-commutativity parameter using…

高能物理 - 理论 · 物理学 2016-09-06 Slimane Zaim

In the weak field and slow motion approximation, the general relativistic field equations are linearized, resembling those of the electromagnetic theory. In a way analogous to that of a moving charge generating a magnetic field, a mass…

广义相对论与量子宇宙学 · 物理学 2013-07-12 Ioannis Haranas , Omiros Ragos , Ioannis Gkigkitzis