DYNAMIC SCALAR TORSION AND AN OSCILLATING UNIVERSE

DOI10.1142/S0217732307025303zbMath1143.83006arXivastro-ph/0612738WikidataQ124830178 ScholiaQ124830178MaRDI QIDQ3499124

James M. Nester, Hwei-Jang Yo

Publication date: 28 May 2008

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

Full work available at URL: https://arxiv.org/abs/astro-ph/0612738

zbMATH Keywords

torsiongravity universe

Mathematics Subject Classification ID

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

Related Items (5)

Poincaré gauge theory with coupled even and odd parity spin-0 modes: Cosmological normal modes ⋮ Neutrino oscillations in cosmological spacetime ⋮ POINCARÉ GAUGE THEORY WITH COUPLED EVEN AND ODD PARITY DYNAMIC SPIN-0 MODES: DYNAMICAL EQUATIONS FOR ISOTROPIC BIANCHI COSMOLOGIES ⋮ Weakly dynamic dark energy via metric-scalar couplings with torsion ⋮ Teleparallel Poincaré cosmology and ΛCDM model

Cites Work

• Cosmological constant -- the weight of the vacuum
• Effects of a torsion field on big bang nucleosynthesis
• HAMILTONIAN ANALYSIS OF POINCARÉ GAUGE THEORY SCALAR MODES
• Gravity from Poincare Gauge Theory of the Fundamental Particles. I: General Formulation
• The cosmological constant and dark energy
• TORSION GRAVITY: A REAPPRAISAL
• HAMILTONIAN ANALYSIS OF POINCARÉ GAUGE THEORY: HIGHER SPIN MODES
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• Physical aspects of the space-time torsion

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