Spatially isotropic homogeneous spacetimes
نویسندگان
چکیده
منابع مشابه
Linear perturbations of spatially locally homogeneous spacetimes
Methods and properties regarding the linear perturbations are discussed for some spatially closed (vacuum) solutions of Einstein’s equation. The main focus is on two kinds of spatially locally homogeneous solution; one is the Bianchi III (Thurston’s H × R) type, while the other is the Bianchi II (Thurston’s Nil) type. With a brief summary of previous results on the Bianchi III perturbations, as...
متن کاملTeleparallel Energy-Momentum Distribution of Spatially Homogeneous Rotating Spacetimes
The energy-momentum distribution of spatially homogeneous rotating spacetimes in the context of teleparallel theory of gravity is investigated. For this purpose, we use the teleparallel version of Moller prescription. It is found that the components of energy-momentum density are finite and well-defined but are different from General Relativity. However, the energy-momentum density components b...
متن کاملStatic Isotropic Spacetimes with Radially Imperfect Fluids
When solving the equations of General Relativity in a symmetric sector, it is natural to consider the same symmetry for the geometry and stress-energy. This implies that for static and isotropic spacetimes, the most general natural stress-energy tensor is a sum of a perfect fluid and a radial imperfect fluid component. In the special situations where the perfect fluid component vanishes or is a...
متن کاملIsotropic cosmological singularities in spatially-homogeneous models with a cosmological constant
We prove well-posedness of the initial value problem for the Einstein equations for spatially-homogeneous cosmologies with data at an isotropic cosmological singularity, for which the matter content is either a cosmological constant with collisionless particles of a single mass (possibly zero) or a cosmological constant with a perfect fluid having the radiation equation of state. In both cases,...
متن کاملHomogeneous and isotropic big rips?
We investigate the way big rips are approached in a fully inhomogeneous description of the space-time geometry. If the pressure and energy densities are connected by a (supernegative) barotropic index, the spatial gradients and the anisotropic expansion decay as the big rip is approached. This behaviour is contrasted with the usual big-bang singularities. A similar analysis is performed in the ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of High Energy Physics
سال: 2019
ISSN: 1029-8479
DOI: 10.1007/jhep01(2019)229