Cited by 213Relativity and Gravitational TheoryCosmology and Gravitation TheoriesAdvanced Differential Geometry Research

General relativity with spin and torsion and its deviations from Einstein's theory

Hehl, Friedrich W., von der Heyde, Paul, Kerlick, G. David·1974·Physical Review D

Abstract

The field equations of general relativity with spin and torsion (${U}_{4}$ theory) are considered to describe correctly the gravitational properties of matter on a microphysical level. By an averaging procedure one arrives at a macroscopic field equation, which under normal matter densities coincides with Einstein's equation of conventional general relativity. For very high matter densities, even if the spin are randomly distributed, Einstein's equation breaks down and ${U}_{4}$ theory must be applied. It is shown how the singularity theorems of Penrose and Hawking must be modified to apply in ${U}_{4}$ theory. All known cosmological models in ${U}_{4}$ theory which prevent singularities are shown to violate an energy condition of a singularity theorem.

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Crossref · 10.1103/physrevd.10.1066

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  • Varying the action with respect to the metric and using the Cartan equations gives the Einstein field equations that relate the curvature of spacetime to the canonical energy-momentum tensor of matter.

    “Varying the action with respect to the metric and using Equation (1) gives the Einstein field equations that relate the curvature of spacetime to the canonical energymomentum tensor of matter s ij ,”

    From UNIVERSE IN A BLACK HOLE IN EINSTEIN–CARTAN GRAVITY (2016) · cites this paper as Hehl et al. 1974

  • If the spin orientation of particles in a spin fluid is random, then the last term on the right-hand side of Equation (6) vanishes after averaging, and the Einstein-Cartan equations for such a spin fluid are equivalent to the Einstein equations for a perfect fluid with effective energy density and pressure.

    “If the spin orientation of particles in a spin fluid is random, then the last term on the right-hand side of Equation (6) vanishes after averaging.Thus, the Einstein-Cartan equations for such a spin fluid are equivalent to the Einstein equations for a perfect fluid with the effective energy density  k s 4 2 and the effective pressure k p s 4 2 (Hehl et al. 1974;Kuchowicz 1978;Gasperini 1986;Bre”

    From UNIVERSE IN A BLACK HOLE IN EINSTEIN–CARTAN GRAVITY (2016) · cites this paper as Hehl et al. 1974

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Authors
Hehl, F. W., von der Heyde, P., & Kerlick, G. D.
Affiliations
Princeton University (US)
Venue
Physical Review D
Published
1974-08-15
Volume
10
Issue
4
Pages
1066-1069
ISSN
0556-2821 (ISSN-L)
OpenAlex
W2171361875
Cited by
213
References
0
Citations by year
2026: 7 · 2025: 14 · 2024: 13 · 2023: 13 · 2022: 3 · 2021: 10 · 2020: 11 · 2019: 13 · 2018: 12 · 2017: 8 · 2016: 4 · 2015: 6 · 2014: 8 · 2013: 7 · 2012: 6
FWCI
7.43
Type
journal article
Language
en
Open access
closed
Locations
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Advanced Differential Geometry Research
Keywords
torsion, spin, averaging procedure, Penrose singularity theorem, energy conditions, cosmological models, singularity avoidance

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