Solutions to a Weak Gravity Quantum Equations and their Significance to the Dark Matter Problem.

Details Solutions to a Weak Gravity Quantum Equations and their Significance to the Dark Matter Problem. Solutions to a Weak Gravity Quantum Equations and their Significance to the Dark Matter Problem.

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006esasp.637e...9e&link_type=abstract

"Proceedings of the EPS-13 Conference "Beyond Einstein – Physics for the 21st Century". 11–15 July 2005. University of Bern, Swi

Physics

A New Theory Of Dark Matter Is Presented In Which Schr&Ouml, Dinger&Rsquo, S Equation Is Applied To Gravitational Potentials On A Macroscopic Scale. Some Of The Stationary State Solutions To This Equation Intrinsically Possess All The Physical Properties Required For Dark Matter, Eliminating The Need To Introduce New Particles Or New Physics. In Particular The Theory Predicts The Existence Of Certain States That Have (1) Negligible Decay Rates Resulting In An Inherent Inability To Gravitationally Collapse O

Scientific paper

A new theory of dark matter is presented in which Schrödinger’s equation is applied to gravitational potentials on a macroscopic scale. Some of the stationary state solutions to this equation intrinsically possess all the physical properties required for dark matter, eliminating the need to introduce new particles or new physics. In particular the theory predicts the existence of certain states that have (1) negligible decay rates resulting in an inherent inability to gravitationally collapse or coalesce and (2) negligible elastic/inelastic scattering rates with particles and electromagnetic radiation. Traditional baryonic particles occupying such eigenstates will be both invisible and weakly interacting. A viable formation and evolutionary scenario for these “eigenstructure” halos can be developed that allows the universe to be “all baryonic” but potentially still consistent with measured Big Bang Nucleosynthesis (BBN) ratios and data from the Wilkinson Microwave Anisotropy Probe (WMAP). This paper outlines the properties, formation, evolution and possible detection of these new dark matter candidates.

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