Abstract
Here approximate expressions for the De Donder-Fock harmonic coordinates are given in the case when kG{sup 2} >> k{sup 2}m{sup 2} and in the case kG{sup 2} << k{sup 2}m{sup 2}, where k is the Newton gravitational constant, G is a scalar constant, m is the mass of a system. Harmonic coordinates appear, in particular, in the Rosen bi metric general relativity and in the Chernikov theory with two connections but one metric if one passes to the Einstein theory. They both contain a generalized condition, which tends to the De Donder harmonic condition in the limiting case. 6 refs., 2 figs.
Citation Formats
Asanov, R A.
Harmonic Coordinates in the Problem on Static Gravitational and Massless Scalar Fields with a Point Source.
JINR: N. p.,
1994.
Web.
Asanov, R A.
Harmonic Coordinates in the Problem on Static Gravitational and Massless Scalar Fields with a Point Source.
JINR.
Asanov, R A.
1994.
"Harmonic Coordinates in the Problem on Static Gravitational and Massless Scalar Fields with a Point Source."
JINR.
@misc{etde_10125369,
title = {Harmonic Coordinates in the Problem on Static Gravitational and Massless Scalar Fields with a Point Source}
author = {Asanov, R A}
abstractNote = {Here approximate expressions for the De Donder-Fock harmonic coordinates are given in the case when kG{sup 2} >> k{sup 2}m{sup 2} and in the case kG{sup 2} << k{sup 2}m{sup 2}, where k is the Newton gravitational constant, G is a scalar constant, m is the mass of a system. Harmonic coordinates appear, in particular, in the Rosen bi metric general relativity and in the Chernikov theory with two connections but one metric if one passes to the Einstein theory. They both contain a generalized condition, which tends to the De Donder harmonic condition in the limiting case. 6 refs., 2 figs.}
place = {JINR}
year = {1994}
month = {Dec}
}
title = {Harmonic Coordinates in the Problem on Static Gravitational and Massless Scalar Fields with a Point Source}
author = {Asanov, R A}
abstractNote = {Here approximate expressions for the De Donder-Fock harmonic coordinates are given in the case when kG{sup 2} >> k{sup 2}m{sup 2} and in the case kG{sup 2} << k{sup 2}m{sup 2}, where k is the Newton gravitational constant, G is a scalar constant, m is the mass of a system. Harmonic coordinates appear, in particular, in the Rosen bi metric general relativity and in the Chernikov theory with two connections but one metric if one passes to the Einstein theory. They both contain a generalized condition, which tends to the De Donder harmonic condition in the limiting case. 6 refs., 2 figs.}
place = {JINR}
year = {1994}
month = {Dec}
}