On the Scalar Theory of Gravitation

1965 ◽  
Vol 33 (2) ◽  
pp. 162-163
Author(s):  
A. L. Harvey
Keyword(s):  
Scalar Theory ◽  
Theory Of Gravitation

COSMOLOGICAL INFLATION IN TENSOR-MULTI-SCALAR THEORY OF GRAVITATION

2018 ◽  
Vol 1 ◽  
pp. 67-81 ◽  
Author(s):  
S.V. Chervon ◽  
◽  
A.S. Kubasov ◽  
K. A. Bolshakova ◽  
◽  
...  
Keyword(s):  
Scalar Theory ◽  
Cosmological Inflation ◽  
Theory Of Gravitation

Planetary orbits for a moving Sun

1969 ◽  
Vol 47 (20) ◽  
pp. 2161-2164 ◽  
Author(s):  
Peter Rastall
Keyword(s):  
The Sun ◽  
Coordinate Systems ◽  
Scalar Theory ◽  
Planetary Orbits ◽  
Theory Of Gravitation

The scalar theory of gravitation is known to be in agreement with observed planetary motions if the Sun is assumed to be stationary with respect to the preferred coordinate systems of the theory. We now assume that the Sun is moving, and we find that, unless its speed is improbably small, there are observable effects on the planetary orbits. The difficulty can be overcome if one assumes that the Newtonian charts are determined by the distribution of matter.

Gravitational Field Equations

1971 ◽  
Vol 49 (6) ◽  
pp. 678-684
Author(s):  
Peter Rastall
Keyword(s):  
Gravitational Field ◽  
Einstein Equations ◽  
Tensor Form ◽  
Field Equations ◽  
Scalar Theory ◽  
Gravitational Fields ◽  
Gravitational Field Equations ◽  
Theory Of Gravitation ◽  
Alternative Field

An earlier, scalar theory of gravitation is assumed to be valid for a class of static gravitational fields. The theory is written in tensor form, and generalized to the case of an arbitrary gravitational field. The interaction between the field and its sources is discussed, and the linearized form of the field equations is derived. Some possible alternative field equations are considered which are compatible with the linearized Einstein equations.

The time-dependent problem in the Jordan-Brans-Dicke tensor-scalar theory of gravitation

Astrophysics ◽  
1994 ◽  
Vol 37 (3) ◽  
pp. 288-296
Author(s):  
G. G. Arutyunyan ◽  
V. V. Papoyan ◽  
V. N. Pervushin ◽  
M. B. Sheftel'
Keyword(s):  
Time Dependent ◽  
Scalar Theory ◽  
Theory Of Gravitation ◽  
Time Dependent Problem

AN APPROACH TO A THEORY OF GRAVITATION

1960 ◽  
Vol 38 (8) ◽  
pp. 975-982 ◽  
Author(s):  
Peter Rastall
Keyword(s):  
Space Time ◽  
Red Shift ◽  
Additive Constant ◽  
The Sun ◽  
Field Equations ◽  
Scalar Theory ◽  
Theory Of Gravitation ◽  
Bending Of Light

The form of the space–time metric in a scalar theory of gravitation follows from the assumption that the potential is arbitrary to the extent of an additive constant. No field equations are needed. Expressions are found for the gravitational red shift, the perihelion motion of a planet, and the bending of light by the sun. From the observed values of these quantities one can determine the metric and the potential due to a gravitating mass.

COSMOLOGICAL INFLATION IN TENSOR-MULTI-SCALAR THEORY OF GRAVITATION

2018 ◽  
Vol 1 ◽  
pp. 50-65 ◽  
Author(s):  
S.V. Chervon ◽  
◽  
A.S. Kubasov ◽  
K. A. Bolshakova ◽  
◽  
...  
Keyword(s):  
Scalar Theory ◽  
Cosmological Inflation ◽  
Theory Of Gravitation
Sign in / Sign up

Export Citation Format

Share Document