Teoretičeskaâ i matematičeskaâ fizika, Tome 111 (1997) no. 1, pp. 144-148
Citer cet article
V. I. Denisov. Analysis of the solution properties of the relativistic theory of gravitation in the vicinity of a singular sphere. Teoretičeskaâ i matematičeskaâ fizika, Tome 111 (1997) no. 1, pp. 144-148. http://geodesic.mathdoc.fr/item/TMF_1997_111_1_a10/
@article{TMF_1997_111_1_a10,
author = {V. I. Denisov},
title = {Analysis of the solution properties of the relativistic theory of gravitation in the vicinity of a singular sphere},
journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
pages = {144--148},
year = {1997},
volume = {111},
number = {1},
language = {ru},
url = {http://geodesic.mathdoc.fr/item/TMF_1997_111_1_a10/}
}
TY - JOUR
AU - V. I. Denisov
TI - Analysis of the solution properties of the relativistic theory of gravitation in the vicinity of a singular sphere
JO - Teoretičeskaâ i matematičeskaâ fizika
PY - 1997
SP - 144
EP - 148
VL - 111
IS - 1
UR - http://geodesic.mathdoc.fr/item/TMF_1997_111_1_a10/
LA - ru
ID - TMF_1997_111_1_a10
ER -
%0 Journal Article
%A V. I. Denisov
%T Analysis of the solution properties of the relativistic theory of gravitation in the vicinity of a singular sphere
%J Teoretičeskaâ i matematičeskaâ fizika
%D 1997
%P 144-148
%V 111
%N 1
%U http://geodesic.mathdoc.fr/item/TMF_1997_111_1_a10/
%G ru
%F TMF_1997_111_1_a10
The analysis of the properties of static spherical symmetric metric of the relativistic theory of gravitation in the vicinity of a singular sphere is done. It is shown that a massive particle in the nongeodesical radial motion may reach this sphere and be remained there in the rest. Basing on this property, it is inferred that the sphere formed by the massive particles can serve as the source of a singular metic in the relativistic theory of gravitation.
