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Treatment of a static spherically symmetric matter distribution on the basis of the projective unified field theory
Author(s) -
Avakian R. M.,
Chubarian E. V.,
Sarkissian A. V.,
Schmutzer E.
Publication year - 1990
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.2113110604
Subject(s) - physics , neutron star , basis (linear algebra) , compact star , distribution (mathematics) , projective test , dense matter , theoretical physics , field (mathematics) , order (exchange) , star (game theory) , classical mechanics , mathematical analysis , pure mathematics , geometry , mathematics , astrophysics , finance , economics
In order to confront the Projective Unified Field Theory with physical experience it is appropriate to apply this theory also to astrophysical objects, for mathematical reasons in particular to a static spherically symmetric matter distribution as a rough model for a star (e.g. neutron star or another exotic compact object). The problem mentioned is treated here as far as possible analytically in order to prepare the basis for the numerical approach.