[astro-ph/0701358] Dark Matter in an n-Space Expanding Universe

[astro-ph/0701358] Dark Matter in an n-Space Expanding Universe:



"The total number of degrees of freedom of a d-dimensional body in n-space is derived so that equipartition of energy may be applied to a possibly n-dimensional early universe. A comparison is made of a range of proposals to include free and bound black holes as either a small component or the dominant constituent of dark matter in the universe. The hypothesis that dark matter consists in part of atomic gravitationally bound primordial black holes is closely examined in 3-space, as well as in n-space; and the Chavda and Chavda holeum hypothesis is found to be flawed. Blackbody and Hawking radiation are generalized to n-space, and Hawking radiation is shown to be simply proportional to the black hole density. The importance of quantum gravity in understanding the role of early universe dark matter is undermined because present approaches to a theory of quantum gravity violate the equivalence principle. A general heuristic proof for geodesics on an expanding hypersphere is presented. Classical limits of Einstein's General Relativity are considered. A novel approach to the accelerated expansion of the universe is discussed. An anomalous surprising aspect of 4-space is demonstrated."

This assumes negligible Hawking radiation

As 95% of the mass of the universe, LBH essentially hold the universe together gravitationally, and their directed radiation contributes to its accelerated expansion. That many LBH doing Hawking Radiation would fry the universe. Unlike LBH that Hawking radiate, my LBH are long-lived because in my model of Gravitational Tunneling Radiation (GTR) they radiate much, much less and the radiation is beamed

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