Cosmic Acceleration and Modified Gravity
arXiv:astro-ph/0607510 · doi:10.1142/S0218271807011723
Abstract
I briefly discuss some attempts to construct a consistent modification to General Relativity (GR) that might explain the observed late-time acceleration of the universe and provide an alternative to dark energy. I mention the issues facing extensions to GR, illustrate these with two specific examples, and discuss the resulting observational and theoretical obstacles. This article comprises an invited talk at the NASA workshop {\it From Quantum to Cosmos: Fundamental Physics Research in Space}
12 pages, 1 figure. Invited talk at the NASA workshop - From Quantum to Cosmos: Fundamental Physics Research in Space, May 21-24 2006
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Cited by in corpus (15)
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- Accelerating Universe in Modified Theories of Gravity
- Standard Cosmological Evolution in a Wide Range of f(R) Models
- Ghost dark energy in model of gravity
- Energy conditions in the theory of gravity
- Observational Signatures: Shadow cast by the effective metric of photons for black holes with rational non-linear electrodynamics
- Geometrical Diagnostics for Generalized Chaplygin Gas
- Standard Cosmological Evolution in f(R) Model to Kaluza Klein Cosmology
- Holographic Dark Energy Like in Gravity
- Probing Einstein-Maxwell-Scalar Black hole via Thin Accretion Disks and Shadows with EHT Observations of M87* and Sgr A*
- Cosmic Acceleration from Causal Backreaction with Recursive Nonlinearities
- Inflation constraints for classes of f(R) models
- Reconstructing f(R) model from Holographic DE: Using the observational evidence
- One-Dimensional Primordial Gravitational Waves In Pure Quadratic Gravity