Dark energy and supermassive black holes
arXiv:astro-ph/0408450 · doi:10.1103/PhysRevD.70.063530
Abstract
This paper deals with a cosmological model in which the universe is filled with tachyon dark energy in order to describe current and future accelerating expansion. We obtain that the simplest condition for the regime of phantom energy to occur in this scenario is that the scalar field be Wick rotated to imaginary values which correspond to an axionic field classically. By introducing analytical expressions for the scale factor or the Hubble parameter that satisfy all constraint equations of the used models we show that such models describe universes which may develop a big rip singularity in the finite future. It is argued that, contrary to a recent claim, the entropy for a universe filled with dark energy is definite positive even on the phantom regime where the universe would instead acquire a negative temperature. It is also seen that, whichever the fate of the tachyonic accelerating universe, it will be stable to any fluctuations of the scalar field, and that since the considered models have all an imaginary sound speed, any overdense regions will undergo an accelerate collapse leading rapidly to formation of giant black holes. Finally the conjecture is advanced that these black holes may be the supermassive black holes that most galaxies harbor at their center.
13 pages, RevTex, accepted for publication in Phys. Rev. D
References in corpus (27)
- Cosmological Results from High-z Supernovae
- Cosmological Dynamics of Phantom Field
- Sudden Future Singularities
- Constructing Phantom Cosmologies from Standard Scalar Field Universes
- Phantom Field and the Fate of Universe
- WMAP and the Generalized Chaplygin Gas
- On the spherical collapse model in dark energy cosmologies
- K-Essential Phantom Energy: Doomsday around the corner?
- You need not be afraid of phantom energy
- deSitter brane universeinduced by phantom and quantum effects
- Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects
- Entropy and universality of Cardy-Verlinde formula in dark energy universe
- Cosmological dynamics of the tachyon with an inverse power-law potential
- Generalized phantom energy
- Testing dark energy beyond the cosmological constant barrier
- Power-law expansion in k-essence cosmology
- Nearly Scale-Invariant Spectrum of Adiabatic Fluctuations May be from a Very Slowly Expanding Phase of the Universe
- Phantom with Born-Infield type Lagrangian
- Phantom k-essence cosmologies
- Axion Phantom Energy
- Phantom Field with O(N) Symmetry in Exponential Potential
- Born-Infeld-type phantom on the brane world
- Achronal cosmic future
- Constructing dark energy models with late time de Sitter attractor
- Wormholes and Ringholes in a Dark-Energy Universe
- Phantom and quantum matter in an Anti-de Sitter Universe
- Sub-Quantum Dark Energy
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- Interacting cosmic fluids in power-law Friedmann-Robertson-Walker cosmological models
- Inflation from D3-brane motion in the background of D5-branes
- Topological Approach to Microcanonical Thermodynamics and Phase Transition of Interacting Classical Spins
- A Quintessentially Geometric Model
- Classical and Quantum Reissner-Nordström Black Hole Thermodynamics and first order Phase Transition
- Tachyon field inspired dark energy and supernovae constraints
- Accretion of Holographic Dark Energy : Dependency only upon Horizon Radius of Expanding Universe
- Inflation driven by single geometric tachyon with D-brane orbiting around NS5-branes