Cosmic de celebration parameter q(Z) dependence upon gravitons? Implications for the DM rocket/ram jet model

Abstract

Cosmic de celebration parameter q(Z) dependence upon gravitons? Implications for the DM rocket/ram jet model abeckwith@uh.edu, beckwith@aibep.org American Institute of Beam Energy propulsion ( life member) PACs: 98.80.Cq, 95.35.+d, 95.30.Sf, 65.40.gd, 11.25.Uv Abstract In the 12th Marcel Grossmann Meeting, July 9, 2009, the author raised the issue of whether early graviton production could affect non-Gaussian contributions to DM density profiles. Another issue to consider, is if or not gravitons with mass affect DM profiles, but could also impact the cosmic acceleration of the universe, leading to an increase of acceleration one billion years ago, in a manner usually attributed to DE. Following Marcio E. S. Alves, Oswaldo D. Miranda, Jose C. N. de Araujo, 2009 in an article brought to the attention to the author by Christian Corda, the author, using his modification of Friedman equations, incorporating some brane models to allow for additional dimensions found that there is, for low graviton

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@inproceedings{Gromann2009CosmicDC, title={Cosmic de celebration parameter q(Z) dependence upon gravitons? Implications for the DM rocket/ram jet model}, author={Marcel Gro\ssmann and Marcio E. S. Alves and Oswaldo D. Miranda and Jos{\'e} Carlos N. de Araujo and Marcell Grossman and Karsten Jedamzik and Martin Lemoine}, year={2009} }