摘要:

A Lorentz-invariant theory of gravitation is examined in which the field variable is a scalar in the sense of the four-dimensional tensor calculus. The Kepler-motion has the same form as in Nordström's theory and differs accordingly from the vector theory. The perihelion motion is of the same absolute value as in the vector theory, and hence much too small in comparison with the experimental value for the planet Mercury, and moreover of the wrong sign. The influence of radiation damping is discussed in a second paper which will be published shortly.

ISSN:0002-9505    

DOI:10.1119/1.1934129

出版商:American Association of Physics Teachers    

年代:1956

数据来源: AIP

ISSN:0002-9505    

DOI:10.1119/1.1934131

出版商:American Association of Physics Teachers    

年代:1956

数据来源: AIP

ISSN:0002-9505    

DOI:10.1119/1.1934133

出版商:American Association of Physics Teachers    

年代:1956

数据来源: AIP

ISSN:0002-9505    

DOI:10.1119/1.1934134

出版商:American Association of Physics Teachers    

年代:1956

数据来源: AIP

ISSN:0002-9505    

DOI:10.1119/1.1934135

出版商:American Association of Physics Teachers    

年代:1956

数据来源: AIP

ISSN:0002-9505    

DOI:10.1119/1.1934137

出版商:American Association of Physics Teachers    

年代:1956

数据来源: AIP

ISSN:0002-9505    

DOI:10.1119/1.1934138

出版商:American Association of Physics Teachers    

年代:1956

数据来源: AIP