Cosmology with scalar–Euler form coupling

DOI10.1088/0264-9381/30/13/135003zbMath1273.83199arXiv1301.0821OpenAlexW2094950708MaRDI QIDQ2845903

Adolfo Toloza, Jorge Zanelli

Publication date: 3 September 2013

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1301.0821

zbMATH Keywords

torsioncosmologyEuler 4-formFriedmann-Robertson-Walker-Lemaître modelJackiw-Teitelboim action

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)

Related Items (8)

Wave operators, torsion, and Weitzenböck identities ⋮ Mimetic Einstein-Cartan-Sciama-Kibble (ECSK) gravity ⋮ n   +  1 formalism of f (Lovelock) gravity ⋮ A black hole solution in conformal supergravity ⋮ Some cosmological models coming from gravitational theories having torsional degrees of freedom ⋮ Cosmological dark matter amplification through dark torsion ⋮ Gauged Wess-Zumino-Witten actions for generalized Poincaré algebras ⋮ Non-minimally coupled scalar field cosmology with torsion

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