Dark Energy from Brane-world Gravity
arXiv:astro-ph/0602415 · doi:10.1088/1742-6596/68/1/012046 10.1007/978-3-540-71013-4_11
Abstract
Recent observations provide strong evidence that the universe is accelerating. This confronts theory with a severe challenge. Explanations of the acceleration within the framework of general relativity are plagued by difficulties. General relativistic models require a "dark energy" field with effectively negative pressure. An alternative to dark energy is that gravity itself may behave differently from general relativity on the largest scales, in such a way as to produce acceleration. The alternative approach of modified gravity also faces severe difficulties, but does provide a new angle on the problem. This review considers an example of modified gravity, provided by brane-world models that self-accelerate at late times.
Based on a talk at the 3rd Aegean Summer School, Chios, September 2005
References in corpus (25)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Quantum Nature of the Big Bang: Improved dynamics
- Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
- Conditions for the cosmological viability of f(R) dark energy models
- Solar System constraints to general f(R) gravity
- The shape of the SDSS DR5 galaxy power spectrum
- Observational constraints on self-accelerating cosmology
- The acceleration of the universe and the physics behind it
- The Cosmological Constant and the String Landscape
- Mimicking Dark Energy with Lemaitre-Tolman-Bondi Models: Weak Central Singularities and Critical Points
- No-go theorem for k-essence dark energy
- Non-linear interactions in a cosmological background in the DGP braneworld
- Constraints on backreaction in dust universes
- The Possibility of Cosmic Acceleration via Spatial Averaging in Lemaitre-Tolman-Bondi Models
- The Limits of Extended Quintessence
- Dark Energy: Recent Developments
- Cosmic Perturbations Through the Cyclic Ages
- Cosmological Surprises from Braneworld models of Dark Energy
- Primordial inflation explains why the universe is accelerating today
- Why Does Gravity Ignore the Vacuum Energy?
- Accelerating Universe via Spatial Averaging
- Brane-world cosmology
- Cosmological Acceleration: Dark Energy or Modified Gravity?
- Illuminating the dark ages of the universe: the exact backreaction in the SFRW model and the acceleration of the universe
Cited by in corpus (8)
- The General Very Special Relativity in Finsler Cosmology
- Thermodynamics and classification of cosmological models in the Horava-Lifshitz theory of gravity
- Friedmann Robertson-Walker model in generalised metric space-time with weak anisotropy
- DM: Observational constraints on unified dark matter with constant speed of sound
- Constraining the evolution of dark energy with type Ia supernovae and gamma-ray bursts
- 7D Randall-Sundrum cosmology, brane-bulk energy exchange and holography
- Colliding branes and formation of spacetime singularities in string theory
- Orbifold Branes in the Compactification of type II string on and their cosmological applications