Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..42..285w&link_type=abstract
Astrophysics and Space Science, vol. 42, July 1976, p. 285-330. Research supported by the Science Research Council.
Astronomy and Astrophysics
Astrophysics
Astronomical Models, Cosmology, Density Distribution, Hierarchies, Relativity, Universe, Einstein Equations, Equations Of Motion, Hubble Diagram, Maxwell-Boltzmann Density Function, Schwarzschild Metric
Scientific paper
The work is an attempt to apply Einstein's field equations in the tractable form given by Podurets (1964) and Misner and Sharp (1964) for a spherically symmetric continuous medium, to superdense bodies and hierarchical continuous cosmology. A central question examined is the conditions under which the step-like density profile of a practical hierarchy can be approximated by a smooth function. It is shown that the notion of a semicontinuous hierarchy would not look asymmetric and anisotropic to an observer on the edge of a given system. The discussion considers the application of the Einstein field equations to an extended cosmological medium, showing how the Hubble parameter is defined, how a finite but very small intergalactic pressure is unavoidable, and what time scales and mass-loss rates are expected in the hierarchy. The metric coefficients for any superdense body are derived and applied to determine the baryon number of a superdense object. The dynamical behavior of a superdense body leads to predictions of energy-loss rates and luminosity.
No associations
LandOfFree
Expanding and superdense astrophysical systems in general relativistic hierarchical cosmology does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Expanding and superdense astrophysical systems in general relativistic hierarchical cosmology, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Expanding and superdense astrophysical systems in general relativistic hierarchical cosmology will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-938280