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An additional production mechanism for the diffuse x-ray background

Published online by Cambridge University Press:  17 July 2013

Allan D. Ernest ,
Matthew P. Collins  and
Graeme L. White
Allan D. Ernest
Affiliation:
Faculty of Science, Charles Sturt University, Wagga Wagga, NSW, 2678Australia email: aernest@csu.edu.au
Matthew P. Collins
Affiliation:
Faculty of Science, Charles Sturt University, Wagga Wagga, NSW, 2678Australia email: aernest@csu.edu.au
Graeme L. White
Affiliation:
Faculty of Science, Charles Sturt University, Wagga Wagga, NSW, 2678Australia email: aernest@csu.edu.au
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Abstract

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We propose a mechanism that contributes energy and particles to the diffuse x-ray halos of galaxies and clusters, based on the dark quantum states of large-scale gravity wells.

Keywords

X-rays: galaxies: clustersgalaxies: halos
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 267
Copyright
Copyright © International Astronomical Union 2013 

References

Ernest, A. D. 2009, J. Phys A: Math. Theor., 42, 115207Google Scholar
Ernest, A. D. 2012, in: Cotaescu, I. (ed.), Advances in Quantum Theory (InTech), p. 221Google Scholar
Nesvizhevsky, V. V., Borner, H. G., & Petukhov, A. K. 2003, Nature, 415, 297Google Scholar