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Halo formation and evolution: unification of structure and physical properties

Published online by Cambridge University Press:  09 May 2016

Allan D. Ernest  and
Matthew P. Collins
Allan D. Ernest
Affiliation:
Charles Sturt University, Locked Bag 588, Wagga Wagga, Australia, 2678 email: [email protected]
Matthew P. Collins
Affiliation:
Charles Sturt University, Locked Bag 588, Wagga Wagga, Australia, 2678 email: [email protected]
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Abstract

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The assembly of matter in the universe proliferates a wide variety of halo structures, often with enigmatic consequences. Giant spiral galaxies, for example, contain both dark matter and hot gas, while dwarf spheroidal galaxies, with weaker gravity, contain much larger fractions of dark matter, but little gas. Globular clusters, superficially resembling these dwarf spheroidals, have little or no dark matter. Halo temperatures are also puzzling: hot cluster halos contain cooler galaxy halos; dwarf galaxies have no hot gas at all despite their similar internal processes. Another mystery is the origin of the gas that galaxies require to maintain their measured star formation rates (SFRs). We outline how gravitational quantum theory solves these problems, and enables baryons to function as weakly-interacting-massive-particles (WIMPs) in Lambda Cold Dark Matter (LCDM) theory. Significantly, these dark-baryon ensembles may also be consistent with primordial nucleosynthesis (BBN) and cosmic microwave background (CMB) anisotropies.

Keywords

halo formation and evolutiondark mattergravitational quantum theory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Issue S317: The General Assembly of Galaxy Halos: Structure, Origin and Evolution , August 2015 , pp. 298 - 299
Copyright
Copyright © International Astronomical Union 2016 

References

Carr, B. 1975, ApJ, 201, 1CrossRefGoogle Scholar
Ernest, A. D. 2006, in Val Blain, J. (ed.), Dark Matter: New Research, (New York: Nova) p. 91Google Scholar
Ernest, A. D. 2009, J. Phys. A: Math. Gen. 42 115207, 115208Google Scholar
Ernest, A. D. & Collins, M. P. 2014, AIP Congress, 7-11 Dec., 2014 Canberra, AustraliaGoogle Scholar
Jenke, T., Geltenbort, P., Lemmel, H., & Abele, H. 2011, Nature Phys, 7, 468Google Scholar