Researchers generalize cosmological models using Finsler geometry.
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Classifies cosmological Finsler spacetimes, finding viable non-stationary models.
The Weyl curvature hypothesis of Penrose attempts to explain the high homogeneity and isotropy, and the very low entropy of the early universe, by conjecturing the vanishing of the Weyl tensor at the Big-Bang singularity. In previous papers it has been proposed an equivalent form of Einstein's equation, which extends i…
The polynomial affine model of gravity is explored in 3D, focusing on cosmological solutions.
The paper investigates the singularity and extendibility of inflationary spacetimes.
The paper examines isotropic cosmological space-times with changing sectional curvature.
Study investigates Einstein flow stability and convergence with matter sources.
New findings show cosmological constant as initial condition for non-isotropic spacetimes.
The universe's shape and size are determined in general cosmological models.
Study classifies moduli spaces of spin connections on 3D homogeneous spaces.
We consider instanton solutions of Euclidean Horava-Lifshitz gravity in four dimensions satisfying the detailed balance condition. They are described by geometric flows in three dimensions driven by certain combinations of the Cotton and Ricci tensors as well as the cosmological-constant term. The deformation curvature…
Study on generalized -Kropina metrics in modified gravity and cosmology.
The paper proves rigidity results for non-positively curved homogeneous Finsler metrics.
Paper proves every homogeneous Landsberg surface is either Riemannian or locally Minkowskian.
Unified cosmological and Einstein polytope theories.
In this paper we consider some properties of the three-dimensional homogeneous SO(2)-isotropic Riemannian manifolds. In particular, we determine the geodesics, the totally geodesic surfaces, the totally umbilical surfaces and the geodesics of the rotational surfaces.
Killing vector fields of a closed homogeneous and isotropic universe are studied. It is shown that in general case there is no time-like Killing vector fields in such a universe. Two exceptional cases are revealed.
In this paper, we show that isotropic Lagrangian submanifolds in a -dimensional strict nearly Kähler manifold are totally geodesic. Moreover, under some weaker conditions, a complete classification of the -isotropic Lagrangian submanifolds in the homogeneous nearly Kähler is also…
We construct a family of flat isotropic non-homogeneous tori in and and find necessary and sufficient conditions for their Hamiltonian minimality.
The closed homogeneous and isotropic universe is considered. The bundles of Weyl and Dirac spinors for this universe are explicitly described. Some explicit formulas for the basic fields and for the connection components in stereographic and in spherical coordinates are presented.
We give a positive answer to the Chavel's conjecture [J. Diff. Geom. 4 (1970), 13-20]: a simply connected rank one normal homogeneous space is symmetric if any pair of conjugate points are isotropic. It implies that all simply connected rank one normal homogeneous space with the property that the isotropy action is var…
In the Friedmann Model of the universe, cosmologists assume that spacelike slices of the universe are Riemannian manifolds of constant sectional curvature. This assumption is justified via Schur's Theorem by stating that the spacelike universe is locally isotropic. Here we define a Riemannian manifold as almost locally…
A proposal is made for what could well be the most natural symmetrical Riemannian spaces which are homogeneous but not isotropic, i.e. of what could well be the most natural class of symmetrical spaces beyond the spaces of constant Riemannian curvature, that is, beyond the spaces which are homogeneous and isotropic, or…
Space-times which allow a slicing into homogeneous spatial hypersurfaces generalize the usual Bianchi models. One knows already that in these models the Bianchi type may change with time. Here we show which of the changes really appear. To this end we characterize the topological space whose points are the 3-dimensiona…
Study compact plane waves, showing they are essentially standard.
The Ricci flow is a parabolic evolution equation in the space of Riemannian metrics of a smooth manifold. To some extent, Einstein equations give rise to a similar hyperbolic evolution. The present text is an introductory exposition to Bianchi-Ricci and Bianchi-Einstein flows, that is, the restricted finitely dimension…
New Galilean spacetimes found as pp-wave reductions.
Geodesic completeness and flow properties of compact Brinkmann spacetimes proven.
In this paper, we first deduce a formula of S-curvature of homogeneous Finsler spaces in terms of Killing vector fields. Then we prove that a homogeneous Finsler space has isotropic S-curvature if and only if it has vanishing S-curvature. In the special case that the homogeneous Finsler space is a Randers space, we giv…
Study proves only origin-centered spheres solve certain curvature problems.
We study the Jacobi osculating rank of geodesics on naturally reductive homogeneous manifolds and we apply this theory to the 3-dimensional case. Here, each non-symmetric, simply connected naturally reductive 3-manifold can be given as a principal bundle over a surface of constant curvature, such that the curvature of …
This paper deals with two aspects of relativistic cosmologies with closed (compact and boundless) spatial sections. These spacetimes are based on the theory of General Relativity, and admit a foliation into space sections S(t), which are spacelike hypersurfaces satisfying the postulate of the closure of space: each S(t…
The abstract proves properties of Berwald spaces with non-zero flag curvature.
Parallel spinors help characterize G2* structures and isotropic forms.
Constructs a Morse-Bott function on symplectic Grassmannians.
Finsler gravity vacuum equation reduces to Ricci vanishing under specific conditions.
Study how past radiation determines present matter in Penrose's cyclic cosmology.
New quasi space forms solve Thurston's geometrical space form problem.
We construct exact sequences of invariant differential operators acting on sections of certain homogeneous vector bundles in singular infinitesimal character, over the isotropic -Grassmannian. This space is equal to , where is , and its standard parabolic subgroup havin…
Researchers find solutions to Einstein equations in higher dimensions.
An invariant description of Bianchi Homogeneous (B.H.) 3-spaces is presented, by considering the action of the Automorphism Group on the configuration space of the real, symmetric, positive definite, matrices. Thus, the gauge degrees of freedom are removed and the remaining (gauge invariant) degrees, are th…
Classifies invariant differential operators on a specific geometric space.
In this paper we are investigating variational homogeneous second order differential equations by considering the questions of how many different variational principles exist for a given spray. We focus our attention on h(2)-variationality; that is, the regular Lagrange function is homogeneous of degree two in the dire…
The paper builds a DPW approach of Willmore surfaces via conformal Gauss maps. As applications, we provide descriptions of minimal surfaces in , isotropic surfaces in and homogeneous Willmore tori via the loop group method. A new example of a Willmore two-sphere in without dual surfaces is …
Simply-connected homogeneous spacetimes for kinematical and aristotelian Lie algebras (with space isotropy) have recently been classified in all dimensions. In this paper, we continue the study of these "maximally symmetric" spacetimes by investigating their local geometry. For each such spacetime and relative to expon…
Bayesian Neural Networks improve precision cosmology from simulations.
Paper introduces a new cosmological volume function and its properties.
We present a generalization of Minkowski's classic theorem on the reconstruction of tetrahedra from algebraic data to homogeneously curved spaces. Euclidean notions such as the normal vector to a face are replaced by Levi-Civita holonomies around each of the tetrahedron's faces. This allows the reconstruction of both s…