GEOMETRICAL ORIGIN OF A COSMOLOGICAL TERM

DOI10.1142/S0218271806009789zbMath1112.83045arXivgr-qc/0605142OpenAlexW2052306735MaRDI QIDQ3434350

Richard T. Hammond

Publication date: 25 April 2007

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0605142

zbMATH Keywords

cosmological term

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Cites Work

• Laboratory bounds for the cosmological term gradient
• A model to explain varying \(\Lambda\), \(G\) and \(\sigma^{2}\) simultaneously
• A cosmological model in Weyl-Cartan spacetime
• From Poincar$eacute$ to affine invariance: how does the Dirac equation generalize?
• A cosmological model in Weyl$ndash$Cartan spacetime: I. Field equations and solutions
• Gravitational theory in Weyl integrable spacetime
• General relativity with spin and torsion: Foundations and prospects

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