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Supernovae, Dark Energy, and the Accelerating Universe

Evolution of the universe, topological change The problem with considering 饾晩饾煈 as a model for the very early universe, is that it is now known that the universe is not closed, is either flat or hyperbolic should the matter density be b · 1967

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physics.gen-ph 1

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2019 1

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Strings, Topological Change and Dark Matter

physics.gen-ph 路 2019-08-12 路 reject 路 novelty 4.0

Dark matter is modeled as same-sign dark charges at the ends of Kalb-Ramond strings, and the standard isothermal halo density profile is shown to be an exact Einstein-Maxwell charged dust solution, though the profile is imposed rather than derived.

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  • Strings, Topological Change and Dark Matter physics.gen-ph 路 2019-08-12 路 reject 路 none 路 ref 5

    Dark matter is modeled as same-sign dark charges at the ends of Kalb-Ramond strings, and the standard isothermal halo density profile is shown to be an exact Einstein-Maxwell charged dust solution, though the profile is imposed rather than derived.