Primordial helium production in ''magnetic'' cosmologies.
Primordial He 3 and deuterium production from magnetic effects during nucleosynthesis epoch of big bang cosmologies
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Primordial He 3 and deuterium production from magnetic effects during nucleosynthesis epoch of big bang cosmologies
Deceleration parameter lower and upper limits for zero pressure big bang cosmological Friedmann models imposed by density parameter, Hubble constant and universe age
Critical test of cosmological pion decay hypothesis for origin of isotropic gamma radiation above 1 MeV
Coordinate system for synthesizing previous work on multifluid cosmologies, investigating noninteracting mixtures of multicomponent fluids
Hamiltonian methods applied to homogeneous cosmological models, obtaining Einstein equations, passing to quantum theory by imposing canonical commutation relations
High energy break in isotropic gamma ray spectrum predicted from critical test of cosmological pion-decay hypothesis
Maxwell equations and equations of massive-vector- meson fields in spatially homogeneous Bianchi cosmologies, obtaining formula for homogeneous EM field
Anisotropic multifluid cosmological models with orthogonal velocity fields
Log S /flux/-log Z /redshift/ diagram for radio galaxies, encouraging steady state cosmology
Cosmology application of mathematical modeling by symbolic computation
Galaxy clusters stabilization by cosmological constant, considering clusters mass discrepancy
Submillimeter background radiation origin possibility from extragalactic discrete sources based on cosmological models
Polynomial Hamiltonian for type VIII and IX vacuum cosmologies, suggesting quantized versions involving fluctuations of 3-space signature and topology
Brans-Dicke cosmologies in arbitrary units, deriving power law solutions in flat Friedmann space
Exact solutions to radiation-filled Brans-Dicke cosmologies, using Robertson-Walker metric
Following the big-bang baryon symmetric cosmology of Omnes, the redshift was calculated to be on the order of 500-600. It is show that, at these redshifts, annihilation pressure at the boundaries between regions of matter and antimatter drives large scale supersonic turbulence which can trigger galaxy formation. This picture is consistent with the gamma-ray background observations discussed previously. Gravitational binding of galaxies then occurs at a redshift of about 70, at which time vortical turbulent velocities of about 3 x 10 to the 7th power cm/s lead to angular momenta for galaxies comparable with measured values.
Initial results of a detailed calculation of the cosmological gamma-ray spectrum from matter-antimatter annihilation in the universe. The similarity between the calculated spectrum and the present observations of the gamma-ray background spectrum above 1 MeV suggests that such observations may be evidence of the existence of antimatter on a large scale in the universe.
Additional quantitative and revealing arguments are given in favor of author's previous suggestion (1971) that the introduction of pressure results in a decrease in the theoretical upper bound on the time variation of G, as predicted by the Brans-Dicke theory (1961) for Friedmann-type expanding cosmologies in flat space, and that this suggestion holds in curved spaces as well. Moreover, it is shown that the curvature contribution to G is of the same order of magnitude as the flat space contribution and adds to it or subtracts from it for positive or negative curvatures respectively.