Metastable dark energy
arXiv:1611.00428 · doi:10.1016/j.physletb.2016.11.044
Abstract
We build a model of metastable dark energy, in which the observed vacuum energy is the value of the scalar potential at the false vacuum. The scalar potential is given by a sum of even self-interactions up to order six. The deviation from the Minkowski vacuum is due to a term suppressed by the Planck scale. The decay time of the metastable vacuum can easily accommodate a mean life time compatible with the age of the universe. The metastable dark energy is also embedded into a model with symmetry. The dark energy doublet and the dark matter doublet naturally interact with each other. A three-body decay of the dark energy particle into (cold and warm) dark matter can be as long as large fraction of the age of the universe, if the mediator is massive enough, the lower bound being at intermediate energy level some orders below the grand unification scale. Such a decay shows a different form of interaction between dark matter and dark energy, and the model opens a new window to investigate the dark sector from the point-of-view of particle physics.
15 pages, 3 figures, references added. Accepted for publication in PLB
References in corpus (63)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Planck 2013 results. XVI. Cosmological parameters
- Dynamics of dark energy
- Cosmological Imprint of an Energy Component with General Equation of State
- Big-Bang Nucleosynthesis
- 4D Gravity on a Brane in 5D Minkowski Space
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- A Model of Holographic Dark Energy
- Coupled Quintessence
- Accelerated expansion of the universe driven by tachyonic matter
- Cosmology with Ultra-light Pseudo-Nambu-Goldstone Bosons
- Entropy Bounds and Dark Energy
- Holographic dark energy and cosmic coincidence
- Transition of the dark energy equation of state in an interacting holographic dark energy model
- Interacting Quintessence
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Cosmology with tachyon field as dark energy
- Interacting quintessence solution to the coincidence problem
- Interacting Dark Matter and Dark Energy
- The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
- Quintessence and Supergravity
- Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
- Constraints on the interacting holographic dark energy model
- Vector Field Models of Inflation and Dark Energy
- Thermodynamics of an accelerated expanding universe
- Coupled dark energy: Towards a general description of the dynamics
- Inflation and late-time cosmic acceleration in non-minimal Maxwell- gravity and the generation of large-scale magnetic fields
- keV sterile neutrino dark matter in gauge extensions of the standard model
- Warm Dark Matter in Low Scale Left-Right Theory
- Minimal Supersymmetric Left-Right Model
- Testing the Interaction between Dark Energy and Dark Matter with Planck Data
- Thermodynamical description of the interaction between holographic dark energy and dark matter
- Cosmological Evolution of Interacting Phantom Energy with Dark Matter
- Interacting Phantom Energy
- Quintessence models in Supergravity
- Quantization and renormalization of the manifest left-right symmetric model of electroweak interactions
- Evidence for interacting dark energy from BOSS
- A Field Theory Model for Dark Matter and Dark Energy in Interaction
- Minimal Left-Right Symmetric Dark Matter
- A W' boson near 2 TeV: predictions for Run 2 of the LHC
- Quantum Field Theory of Interacting Dark Matter/Dark Energy: Dark Monodromies
- Sneutrino Dark Matter in Gauged Inverse Seesaw Models for Neutrinos
- Holographic dark energy from minimal supergravity
- Dark energy, the electroweak vacua and collider phenomenology
- Cosmological Evolution of Interacting Dark Energy Models with Mass Varying Neutrinos
- Metastable Dark Energy with Radioactive-like Decay
- Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
- Phenomenology of left-right symmetric dark matter
- Massive Photon and Dark Energy
- Dark energy, the colored anti-de Sitter vacuum, and LHC phenomenology
- Quintessence with Yukawa Interaction
- Dynamical analysis for a vector-like dark energy
- A Model for Dark Energy decay
- Dark matter and LHC phenomenology in a left-right supersymmetric model
- The transition of equation of state of effective dark energy in the DGP model with bulk contents
- Possible solution to the main cosmological constant problem
- Reconsidering a higher-spin-field solution to the main cosmological constant problem
- Vector-field model with compensated cosmological constant and radiation-dominated FRW phase
- Mixed Dark Matter in Left-Right Symmetric Models
- SU(2)SU(2) minimal dark matter with 2 TeV
- Cosmological tracking solution and the Super-Higgs mechanism
- Supersymmetric Left-Right Model of Radiative Neutrino Mass with Multipartite Dark Matter
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- Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the - plane
- J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
- Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
- Fractional dark energy
- The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
- A note on interacting holographic dark energy with a Hubble-scale cutoff
- False vacuum decay in kink scattering
- Cosmological implications of the transition from the false vacuum to the true vacuum state
- Quantum mechanical look at the radioactive-like decay of metastable dark energy
- Cosmological perturbations and dynamical analysis for interacting quintessence
- Constraints on interacting dark energy revisited: implications for the Hubble tension
- Interacting dark energy in the dark model
- Dark energy, scalar singlet dark matter and the Higgs portal
- Constraints on Metastable Dark Energy Decaying into Dark Matter
- The KSVZ Axion Model with Quasi-Degenerate Minima: A Unified Model for Dark Matter and Dark Energy
- Cosmology from a running vacuum model driven by a scalar field
- A universe born in a metastable false vacuum state needs not die
- Extended Metastable Dark Energy
- Cosmological "constant" in a universe born in the metastable false vacuum state