Showing papers on "Big Rip published in 1968"
TL;DR: Einstein equations with flat homogeneous hypersurfaces including effects of viscosity in radiation and anisotropic pressures were studied in this paper, where the authors considered flat hypersurface models with flat surfaces.
Abstract: Einstein equations with flat homogeneous hypersurfaces including effects of viscosity in radiation and anisotropic pressures
694 citations
114 citations
TL;DR: In this paper, the authors discuss baryon inhomogeneity in early high density high temperature universe, and show that matter excess over antimatter occurs in early homogeneous high temperature universes.
Abstract: Matter excess over antimatter in early high density high temperature universe, discussing baryon inhomogeneity
39 citations
10 citations
4 citations
Book•
22 Jan 1968
TL;DR: Hawkin's discovery that the vast bulk of the universe is in the form of primordial black holes which had their genesis within the first instant of creation is described in this article.
Abstract: This work describes Dr Hawkin's discovery that the vast bulk of the universe is in the form of primordial black holes which had their genesis within the first instant of creation. It is a key cosmological breakthrough that draws together the most significant insights of our era into a comprehensive view of the universe. Dr Hawkins started an investigation 20 years ago into 300 quasars - the brightest objects in the universe - and why they change in brightness. Calculations based on his research showed that 99 percent of the universe is made up of dark objects that cannot be directly seen - some as big as the planet Jupiter, others mini black holes (imploded stars). Their discovery has solved the mystery of what consitutes as much as 99 percent of the universe's mass.
2 citations
01 Apr 1968
1 citations
01 Jan 1968
TL;DR: In this article, the authors examined the amount of knowledge we can have about states of objects at other places and temporal instants and the degree of its reliability, and how we can reach a conclusion about the size and geometry of our universe.
Abstract: IN Chapter 6 we considered what it meant to say of Space that it had a certain geometry, was finite or infinite and, if finite, had a certain volume. In Chapter 9 and in the last two chapters we have examined the amount of knowledge we can have about states of objects at other places and temporal instants and the degree of its reliability. We are now in a position to examine how we can reach a conclusion about the size and geometry of our Universe.