Hostname: page-component-77c89778f8-cnmwb Total loading time: 0 Render date: 2024-07-17T01:04:26.635Z Has data issue: false hasContentIssue false
  • English
  • Français

A solution to unconstrained Einstein’s equations for a relativistic radiation sphere

Published online by Cambridge University Press:  23 June 2017

Luboš Neslušan Open the ORCID record for Luboš Neslušan [Opens in a new window]
Luboš Neslušan*
Affiliation:
Astronomical Institute, Slovak Academy of Sciences, 05960 Tatranská Lomnica, Slovakia; email: ne@ta3.sk
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We describe an application of a solution to unconstrained Einstein’s field equations (Ni, 2011) as a qualitative model for a relativistic radiation sphere, an object that may resemble a quasar with an extended galactic-scale ‘corona’ that resembles behaviors explained by dark matter.

Keywords

Relativity(galaxies:) quasars: general(cosmology:) dark matter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 355 - 356
Copyright
Copyright © International Astronomical Union 2017 

References

Einstein, A. 1915, Sitzungsberichte der Preussischen Akad. der Wissenschaften zu Berlin, p. 844Google Scholar
Einstein, A. 1916, Annalen der Physik, 354, 769 Google Scholar
Neslušan, L. 2015, J. Modern Phys., 6, 2164 CrossRefGoogle Scholar
Ni, J. 2011, Sci. China: Phys. Mechan. Astron., 54, 1304 Google Scholar
Oppenheimer, J. R. & Volkoff, G. M. 1939, Phys. Rev., 55, 374 CrossRefGoogle Scholar