Relativistic cosmology.
Cosmologies based on Robertson-Walker universe model, discussing pseudo-Newtonian, general relativistic and Friedman models
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Cosmologies based on Robertson-Walker universe model, discussing pseudo-Newtonian, general relativistic and Friedman models
Relativity theory and astrophysics - Conference, Ithaca, July-August 1965, Volume 1, Relativity and cosmology
Cosmology models in light of transport equation assuming relativity and conventional physical laws, noting densities inconsistent with closure
Cosmological implications of Brans-Dicke scalar- tensor theory, discussing primordial elements abundances
Three sphere backgrounds for space section of Taub cosmological solution, discussing wave background separation model
Isotropic 1-100 Mev gamma radiation and cosmic ray detection of cosmological significance
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