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A natural scalar field in the Einstein gravitational theory

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Publication:1149650
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DOI10.1007/BF00756174zbMath0454.53024MaRDI QIDQ1149650

S. H. Smith

Publication date: 1980

Published in: General Relativity and Gravitation (Search for Journal in Brave)


zbMATH Keywords

Riemann tensorirrotational partpotential reductionsolenoidal part


Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Applications of local differential geometry to the sciences (53B50) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Local Riemannian geometry (53B20)


Related Items

On effective constraints for the Riemann–Lanczos system of equations, A new gravitational energy tensor, On the relativistic extension of the equations of the classical gravitational potential, Third-order tensor potentials for the Riemann and Weyl tensors, Third-order tensor potentials for the Riemann and Weyl tensors. II: Singular solutions, Is the Riemann tensor derivable from a tensor potential?



Cites Work

  • Mach's Principle and a Relativistic Theory of Gravitation
  • The Splitting of the Riemann Tensor
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