Comments on the scalar-tensor representation of nonlocally corrected gravity

DOI10.1134/S0202289309030049zbMath1176.83114arXiv0809.4927OpenAlexW2089142473MaRDI QIDQ733893

N. A. Koshelev

Publication date: 19 October 2009

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0809.4927

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items

Ghosts in classes of non-local gravity, Acausality in nonlocal gravity theory, Gravity in the infrared and effective nonlocal models, Initial conditions and degrees of freedom of non-local gravity, Cosmological dynamics and dark energy from nonlocal infrared modifications of gravity, Apparent ghosts and spurious degrees of freedom in non-local theories, Reconciling absence of vDVZ discontinuity with absence of ghosts in nonlocal linearized gravity, Screening of cosmological constant for de Sitter universe in non-local gravity, phantom-divide crossing and finite-time future singularities, SCREENING OF COSMOLOGICAL CONSTANT IN NON-LOCAL COSMOLOGY, A MODIFIED MODEL OF NONLOCALLY CORRECTED GRAVITY: COSMOLOGY AND THE NEWTONIAN LIMIT, Nonlocal gravity. Conceptual aspects and cosmological predictions

Cites Work

• Modified non-local-\(F(R)\) gravity as the key for the inflation and dark energy
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Cosmological parameters from supernova observations: A critical comparison of three data sets
• The cosmological constant problem