Statistics – Computation
Scientific paper
Aug 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.194....1t&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 194, no. 1, p. 1-129.
Statistics
Computation
4
Active Galactic Nuclei, Celestial Mechanics, Computational Astrophysics, Neutron Stars, Accretion Disks, Astronomical Models, Baryons, Equilibrium Equations, Numerical Integration
Scientific paper
Numerical methods are discussed for characterizing the internal structure of supermassive compact celestial bodies with attention given to the equilibrium configurations of baryonic and neutron protomatter. The methods by Ter-Kazarian (1989) and Oppenheimer and Volkoff (1939) are shown to yield equivalent descriptions of the ideal degenerated neutron gas in the absence of spatial and temporal distortion. The equations describing the equilibrium configurations of baryonic protomatter (ECBP) are integrated, and stable stationary supermassive cores are shown to form in specific configurations of degenerated ideal neutron gas such as in AGNs with accretion disks. An upper limit is defined for the total masses of equilibrium configurations of 3.5 x 10 exp 8 solar mass. Models are developed for 61 AGNs, and the observed time scales of the flux variations do not contradict the predictions of the proposed methods.
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