Possible theoretical limits on holographic quintessence from weak gravity conjecture

Abstract

The holographic dark energy model is one of the important ways for dealing with the dark energy problems in the quantum gravity framework. In this model, the dimensionless parameter $c$ plays an essential role in determining the evolution of the holographic dark energy. In particular, the holographic dark energy with $c\ge 1$ can be effectively described by a quintessence scalar-field. However, according to the requirement of the weak gravity conjecture the variation of the quintessence scalar-field should be less than the Planck mass, which would give theoretic constraints on the parameters $c$ and ${\Omega }_{m0}$. Therefore, we get the possible theoretical limits on the parameter $c$ for the holographic quintessence model.

LaTex, 13 pages and 4 figures, revised version

References in corpus (79)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Dynamics of dark energy
• The Cosmological Constant and Dark Energy
• The World as a Hologram
• Cosmological parameters from SDSS and WMAP
• Cosmological Imprint of an Energy Component with General Equation of State
• de Sitter Vacua in String Theory
• A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
• Cosmological Constant - the Weight of the Vacuum
• The Case for a Positive Cosmological Lambda-term
• Cosmology and the Fate of Dilatation Symmetry
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• The Cosmological Constant
• An alternative to quintessence
• Phantom Energy and Cosmic Doomsday
• Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
• Hierarchies from Fluxes in String Compactifications
• A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
• A Model of Holographic Dark Energy
• Essentials of k-essence
• Coupled Quintessence
• Effective Field Theory, Black Holes, and the Cosmological Constant
• The String Landscape, Black Holes and Gravity as the Weakest Force
• Dark Energy Constraints from the Cosmic Age and Supernova
• On the Geometry of the String Landscape and the Swampland
• The Second Data Release of the Sloan Digital Sky Survey
• Tachyon Matter
• Accelerated Universe from Gravity Leaking to Extra Dimensions
• Accelerated expansion of the universe driven by tachyonic matter
• Ghost Condensation and a Consistent Infrared Modification of Gravity
• Entropy Bounds and Dark Energy
• Cosmological Evolution of a Quintom Model of Dark Energy
• The Third Data Release of the Sloan Digital Sky Survey
• Braneworld models of dark energy
• CDM Models with a Smooth Component
• Probable Values of the Cosmological Constant in a Holographic Theory
• Constraints on holographic dark energy from type Ia supernova observations
• The Holographic Dark Energy in a Non-flat Universe
• Dark Energy: Vacuum Fluctuations, the Effective Phantom Phase, and Holography
• Dilatonic ghost condensate as dark energy
• Hessence: A New View of Quintom Dark Energy
• Statefinder diagnostic for holographic dark energy model
• Supernova Constraints on a holographic dark energy model
• Statefinder diagnostic for coupled quintessence
• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• Extended Holographic dark energy
• Interacting dark energy, holographic principle and coincidence problem
• Dark Energy and Dark Matter
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• Variable Cosmological Constant as a Planck Scale Effect
• Reconstructing holographic quintessence
• New generalized Chaplygin gas as a scheme for unification of dark energy and dark matter
• Running G and Λat low energies from physics at M_X: possible cosmological and astrophysical implications
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
• Coupled Quintessence in a Power-Law Case and the Cosmic Coincidence Problem
• Statefinder diagnosis for the interacting model of holographic dark energy
• Anthropic Principle Favors the Holographic Dark Energy
• Constraints on the dark energy from holography
• Statefinder diagnosis in a non-flat universe and the holographic model of dark energy
• Testing the running of the cosmological constant with Type Ia Supernovae at high z
• Holographic tachyon model
• Age Problem in the Holographic Dark Energy Model
• The Holographic dark energy reexamined
• Holographic dark energy in a cyclic universe
• Current constraints on interacting holographic dark energy
• Critical comments on the paper "Crossing $\omega =-1$ by a single scalar field on a Dvali-Gabadadze-Porrati brane" by H Zhang and Z-H Zhu [Phys.Rev.D75,023510(2007)]
• Crossing $w=-1$ by a single scalar on a Dvali-Gabadadze-Porrati brane
• Inflation with Holographic Dark Energy
• Constraints on the spectral index for the inflation models in string landscape
• Weak gravity conjecture in the asymptotical dS and AdS background
• Accelerating Universe and Cosmological Perturbation in the Ghost Condensate
• Variable Cosmological Constant model: the reconstruction equations and constraints from current observational data
• Weak gravity conjecture constraints on inflation
• Theoretic Limits on the Equation of State Parameter of Quintessence
• Eternal Chaotic Inflation is Prohibited by Weak Gravity Conjecture

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• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
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• Planck Constraints on Holographic Dark Energy
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• Comparison of dark energy models: A perspective from the latest observational data
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
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• Revisit of the interacting holographic dark energy model after Planck 2015
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• Observational constraints on the interacting Ricci dark energy model
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
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• Cosmological models with Lagrange Multiplier Field
• Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future
• Sandage-Loeb test for the new agegraphic and Ricci dark energy models
• New agegraphic dark energy as a rolling tachyon
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• Couplings between holographic dark energy and dark matter
• Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
• Holographic Dark Energy with Cosmological Constant
• Variable Cosmological Constant model: the reconstruction equations and constraints from current observational data
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• Diagnosing holographic dark energy models with statefinder hierarchy
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• Generalized Holographic Dark Energy and its Observational Constraints
• Strong gravitational lensing constraints on holographic dark energy
• Comparing holographic dark energy models with statefinder
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Cosmological search for sterile neutrinos after Planck 2018
• Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data
• Constraining the interacting dark energy models from weak gravity conjecture and recent observations
• Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• Cosmological constraints on the new holographic dark energy model with action principle
• A Two-field Dilaton Model of Dark Energy
• Theoretical Limits on Agegraphic Quintessence from Weak Gravity Conjecture
• Holographic dilatonic model of dark energy
• Holographic Λ(t)CDM model in a non-flat universe
• Polytropic gas scalar field models of dark energy
• The interacting generalized Ricci dark energy model in non-flat universe
• Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• Quintessence and phantom emerging from the split-complex field and the split-quaternion field
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
• Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature
• Weak Gravity Conjecture and Holographic/Agegraphic Dark Energy