Holographic Foam, Dark Energy and Infinite Statistics
arXiv:gr-qc/0703096 · doi:10.1016/j.physletb.2007.09.052
Abstract
Quantum fluctuations of spacetime give rise to quantum foam, and black hole physics dictates that the foam is of holographic type. Applied to cosmology, the holographic model requires the existence of dark energy which, we argue, is composed of an enormous number of inert ``particles'' of extremely long wavelength. These "particles" necessarily obey infinite statistics in which all representations of the particle permutation group can occur. For every boson or fermion in the present observable universe there could be such "particles". We also discuss the compatibility between the holographic principle and infinite statistics.
12 pages, LaTeX; added references and footnotes; version to appear in Physics Letters B
References in corpus (2)
Cited by in corpus (17)
- A Dark Energy Model Characterized by the Age of the Universe
- Cosmological Constraints on New Agegraphic Dark Energy
- Interacting Agegraphic Dark Energy
- Origin of holographic dark energy models
- Planck priors for dark energy surveys
- Holographic Gas as Dark Energy
- A preliminary analysis of the energy transfer between the dark sectors of the Universe
- Agegraphic dark energy: growth index and cosmological implications
- Fine Structure of Dark Energy and New Physics
- A Comment or two on Holographic Dark Energy
- Entropy and Gravitation: From Black Hole Computers to Dark Energy and Dark Matter
- Coupling q-deformed dark energy to dark matter
- Space-time uncertainty relation from quantum and gravitational principles
- Physics of computation and light sheet concept in the measurement of (4+n)-dimensional spacetime geometry
- Entropy growth in the early universe and confirmation of initial big bang conditions (Why the quark-gluon model is not the best analogy)
- A Possible Approach to Inclusion of Space and Time in Frame Fields of Quantum Representations of Real and Complex Numbers
- Interacting dark matter and q-deformed dark energy non-minimally coupled to gravity