DARK ENERGY AND DARK MATTER IN GENERAL RELATIVITY WITH LOCAL SCALE INVARIANCE

DOI10.1142/S0217732309030060zbMath1168.83339arXiv0810.4421MaRDI QIDQ3395418

Naveen K. Singh, Pavan Kumar Aluri, Pankaj Jain

Publication date: 1 September 2009

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0810.4421

zbMATH Keywords

dark matterscale invariancesymmetry breakingdark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Symmetry breaking in quantum theory (81R40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (5)

(Anti) de Sitter geometry, complex conformal gravity-Maxwell theory from a \(Cl(4, C)\) gauge theory of gravity and grand unification ⋮ STANDARD MODEL WITH COSMOLOGICALLY BROKEN QUANTUM SCALE INVARIANCE ⋮ CONSTRAINTS ON THE COSMOLOGICAL CONSTANT DUE TO SCALE INVARIANCE ⋮ CONFORMAL INVARIANCE IN EINSTEIN–CARTAN–WEYL SPACE ⋮ UNIMODULAR CONSTRAINT ON GLOBAL SCALE INVARIANCE

Cites Work

• Cosmological constant -- the weight of the vacuum
• The cosmological constant and dark energy
• DYNAMICS OF DARK ENERGY
• COSMOLOGICAL SYMMETRY BREAKING, PSEUDO-SCALE INVARIANCE, DARK ENERGY AND THE STANDARD MODEL
• New conformal gauging and the electromagnetic theory of Weyl
• A dynamical symmetry breaking model in Weyl space
• THE VIRGO ALIGNMENT PUZZLE IN PROPAGATION OF RADIATION ON COSMOLOGICAL SCALES
• Oscillatory regime in the multidimensional homogeneous cosmological models induced by a vector field
• Dark matter and dark energy: summary and future directions
• Cosmological Imprint of an Energy Component with General Equation of State
• The cosmological constant problem
• Dilaton-derived quintessence scenario leading naturally to the late-time acceleration of the Universe

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