Is dark energy from cosmic Hawking radiation?
arXiv:0803.1987 · doi:10.1142/S0217732310032469
Abstract
It is suggested that dark energy is the energy of the Hawking radiation from a cosmic horizon. Despite of its extremely low Gibbons-Hawking temperature, this radiation could have the appropriate magnitude and the equation of state to explain the observed cosmological data if there is a Planck scale UV-cutoff, where is the Hubble parameter.
8 pages, 2 figs, revtex, accepted for publication in Modern physics letters
References in corpus (14)
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Fiber-optical analogue of the event horizon
- First Observation of the Greisen-Zatsepin-Kuzmin Suppression
- A Dark Energy Model Characterized by the Age of the Universe
- Dark Energy and Gravity
- Instability of holographic dark energy models
- The Cosmic Horizon
- Probing for dynamics of dark energy and curvature of universe with latest cosmological observations
- Age Problem in the Holographic Dark Energy Model
- Thermodynamical properties of the Universe with dark energy
- Casimir Effect confronts Cosmological Constant
- Dark energy, inflation and the cosmic coincidence problem
- Dark Energy From Vacuum Fluctuations
- Cosmological energy in a thermo-horizon and the first law
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- Gravity as Quantum Entanglement Force
- Temperature upper bound of an ideal gas
- Zero Cosmological Constant and Nonzero Dark Energy from Holographic Principle
- The emergence of gravity as a retro-causal post-inflation macro-quantum-coherent holographic vacuum Higgs-Goldstone field