Physics
Scientific paper
Nov 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006esasp.637e..10e&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
Scientific paper
Understanding the nature and origin of dark matter and dark energy are two of the most challenging problems facing modern cosmology. In recent work by Ernest [1], quantum theory was applied to gravitational potentials to predict ‘dark’ states that might aid in understanding the nature of dark matter. This paper examines whether another quantum phenomena, that of fermionic degeneracy pressure, could be involved with the acceleration of galactic clusters. In this scenario, the presence of a sufficient number of low temperature background neutrinos results in a force between galactic clusters not unlike universal acceleration. This scenario, however requires extending the quantum notion of trapped particles in a box of finite size to one of infinite size, and implies a hypothesis that a fundamental relationship could exist between the average energy and number density of a collection of identical fermionic particles in free space. Low energy fermions such as neutrinos emitted from galaxies could then cause a reaction force as a result of attempting to inject them into a population already consisting of an almost filled set of available states. In this paper the hypothesis is discussed and evaluated.
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