Non-Riemannian cosmology: The role of shear hypermomentum

DOI10.1142/S0219887821501292arXiv2010.00875OpenAlexW3156169186WikidataQ115245297 ScholiaQ115245297MaRDI QIDQ6118709

Damianos Iosifidis

Publication date: 21 March 2024

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

Full work available at URL: https://arxiv.org/abs/2010.00875

zbMATH Keywords

torsionnon-Riemannian geometryshear currentmetric-affine gravitynon-metricitynon-Riemannian cosmologyhypermomentumcosmological hyperfluid

Mathematics Subject Classification ID

Differential geometry (53-XX) Relativity and gravitational theory (83-XX)

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Cites Work

• General teleparallel quadratic gravity
• Metric-affine variational principles in general relativity. II: Relaxation of the Riemannian constraint
• On a model of an unconstrained hyperfluid
• Hyperfluid -- a model of classical matter with hypermomentum
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Exactly solvable connections in metric-affine gravity
• Quantum gravity with torsion and non-metricity
• PERFECT HYPERMOMENTUM FLUID: VARIATIONAL THEORY AND EQUATIONS OF MOTION
• Homogeneous isotropic models in the metric-affine gauge theory of gravity
• Cosmic acceleration with torsion and non-metricity in Friedmann-like Universes
• Projective and amplified symmetries in metric–affine theories
• Ricci-Calculus

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