Results 51 to 60 of about 17,519 (197)
Horizon, homogeneity and flatness problems: do their resolutions really depend upon inflation?
The horizon problem, encountered in cosmology, is derived as such for world models based on Robertson–Walker metric where homogeneity and isotropy of the universe is assumed to begin with and is guaranteed for all epochs.
Ashok K. Singal
doaj +1 more source
Global Dynamics of the Hořava–Lifshitz Cosmological Model in a Non-Flat Universe with Non-Zero Cosmological Constant [PDF]
Fabao Gao, Jaume Llibre
openalex +1 more source
Homogeneity, Flatness and "Large" Extra Dimensions [PDF]
We consider a model in which the universe is the direct product of a (3+1)-dimensional Friedmann, Robertson-Walker (FRW) space and a compact hyperbolic manifold (CHM). Standard Model fields are confined to a point in the CHM (i.e. to a brane).
A. D. Linde +25 more
core +2 more sources
UNIVERSE EVOLUTION IN A 5D RICCI-FLAT COSMOLOGY [PDF]
We use Wetterich's parametrization equation of state (EOS) of dark energy to a 5D Ricci-flat cosmological solution and we assume that the universe contains three major components: matter, radiation and dark energy. By using the relation between the scale factor and the redshift z, we show that the two arbitrary functions contained in the 5D solution ...
Zhang, Chengwu +3 more
openaire +2 more sources
Asymptotic freedom, asymptotic flatness and cosmology [PDF]
Holographic RG flows in some cases are known to be related to cosmological solutions. In this paper another example of such correspondence is provided. Holographic RG flows giving rise to asymptotically-free $ $-functions have been analyzed in connection with holographic models of QCD.
openaire +4 more sources
Cosmology and Conformally Flat Space. II
Not ...
openaire +3 more sources
Cosmology in Conformally Flat Spacetime
A possible solution to cosmological age and redshift-distance difficulties has recently been proposed by applying the appropriate conformally flat spacetime (CFS) coordinates to the standard solution of the field equations in a standard dust model closed universe.
openaire +1 more source
The cluster abundance in flat and open cosmologies [PDF]
Uuencoded package containing LaTeX file (uses mn.sty) plus 7 postscript figures incorporated using epsf. Total length 10 pages. Final version, to appear MNRAS. COBE comparison changed to 4yr data.
Viana, Pedro T P, Liddle, Andrew R
openaire +3 more sources
The majority of satellite galaxies around the Milky Way (MW) show disk-like distributions (the disk of satellites; DoS), which is a small-scale problem of the lambda cold dark matter cosmology.
Chanoul Seo +4 more
doaj +1 more source
Conformally Flat Bulk Tilted Cosmological Model
Conformally flat plane symmetric bulk viscous fluid tilted cosmological model is investigated. We assume that ζθ = K (constant), where ζ is the coefficient of bulk viscosity and θ is the expansion in the model. It has been assumed that the supplementary condition between metric potential as A = B n, where n is constant.
Anita Bagora, Rakeshwar Purohit
openaire +1 more source

