Summary
In this paper I have tried to consider the further effect of the remaining field equations on the solution of the first two field equations of Einstein’s set under the λ-conditions which give rise to the constant values of the scalarK in the second class space-time, obtained in my previous paper. The notations are as usual; followingV. Hlavatt:Geometry of Einstein’s Unified Field Theory.
Riassunto
In questo scritto si è tentato di prendere in considerazione gli ulteriori effetti delle rimanenti equazioni del campo sulla soluzione delle prime due equazioni del campo del gruppo di Einstein con le eondizioni λ che danno luogo a valori costanti dello scalareK nello spazio-tempo di seconda classe, ottenuto in un articolo precedente. Le notazioni sono quelle usuali, secondoV. Hlavatt:Geometry of Einstein’s Unified Theory.
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References
K. Chandra Shekhar:Riv. Mat. Univ. Parma,2, 2 (1963) to appear.
V. Hlavaty:Geometry of Einstein’s Unified Field Theory (Groningen, 1958).
A. Einstein:The Meaning of Relativity, 5th ed.
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Shekhar, K.C. Particular solution of Einstein’s field equations. Nuovo Cim 28, 902–907 (1963). https://doi.org/10.1007/BF02782020
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DOI: https://doi.org/10.1007/BF02782020