The Einsteinian Star Model in Treder's Tetrad Theory of Gravitation | Zendy

Gottlöber S. | Zendy

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The Einsteinian Star Model in Treder's Tetrad Theory of Gravitation

Author(s) -

Gottlöber S.

Publication year - 1981

Publication title -

annalen der physik

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.009

H-Index - 68

eISSN - 1521-3889

pISSN - 0003-3804

DOI - 10.1002/andp.19814930108

Subject(s) - tetrad , physics , gravitation , general relativity , theoretical physics , cluster (spacecraft) , radius , theory of relativity , point particle , star (game theory) , classical mechanics , mathematical physics , astrophysics , computer science , computer security , programming language

By means of a simple star model proposed by E INSTEIN (point‐particle cluster) the collapse behaviour in General Relativety and in T REDER 's [14] Tetrad Theory has been compared. Within both theories the heavy mass of a point‐particle cluster with a fixed radius cannot exceed a critical value. However, contrary to General Relativity, within the framework of T REDER 's Tetrad Theory, for a fixed particle number N , the radius of the cluster is allowed to be arbitrarily small. In this sense, the Tetrad Theory is a collapse‐free relativistic theory of gravitation.

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