Agegraphic Model based on the Generalized Uncertainty Principle

Abstract

Many models of dark energy have been proposed to describe the universe since the beginning of the Big Bang. In this study, we present a new model of agegraphic dark energy ($NADE$) based on the three generalized uncertainty principles $KMM$ (Kempf, Mangan, Mann), Nouicer and $GU{P}^{\ast }$ ( higher orders generalized uncertainty principle).Using the obtained relations from three of types of $GUP$, in the form of three scenarios(Emergent,Intermediate,Logamediate), we consider three different eras of the universe evolution. Also we describe the evolution and expansion of the universe in each subsection. We will plot the obtained relations in these models for better comparatione.

arXiv comment23 pages, 28 figures, Accepted for publication in IJGMMP

References in corpus (53)

• 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
• Cosmological parameters from SDSS and WMAP
• A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
• Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• A Model of Holographic Dark Energy
• The holographic principle
• The Second Data Release of the Sloan Digital Sky Survey
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
• Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
• Entropy Bounds and Dark Energy
• Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints
• Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters
• Purely kinetic k-essence as unified dark matter
• A Dark Energy Model Characterized by the Age of the Universe
• The Microwave Anisotropy Probe (MAP) Mission
• A New Model of Agegraphic Dark Energy
• The Holographic Dark Energy in a Non-flat Universe
• Type Ia Supernova Distances at z > 1.5 from the Hubble Space Telescope Multi-Cycle Treasury Programs: The Early Expansion Rate
• Coupled dark energy: Towards a general description of the dynamics
• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• The Holographic Principle
• Effective Field Theory of Dark Energy: a Review
• A Higher Order GUP with Minimal Length Uncertainty and Maximal Momentum
• Cosmological Constraints on New Agegraphic Dark Energy
• Emergent Universe with Exotic Matter
• Statefinder Diagnosis for Ricci Dark Energy
• Instability of holographic dark energy models
• Instability of agegraphic dark energy models
• Interacting Agegraphic Dark Energy
• Statefinder Diagnostic and w-w' Analysis for the Agegraphic Dark Energy Models without and with Interaction
• Dark Energy: the Cosmological Challenge of the Millennium
• New Type Ia supernova Yields and the Manganese and Nickel Problems in the Milky Way and Dwarf Spheroidal Galaxies
• Dynamics of Logamediate Inflation
• Age Problem in the Holographic Dark Energy Model
• Cosmological implications of Karolyhazy uncertainty relation
• An Uncertainty Relation of Space-Time
• Tachyon dark energy models: dynamics and constraints
• Dark energy exponential potential models as curvature quintessence
• Holographic principle and dark energy
• A Note on Agegraphic Dark Energy
• New agegraphic dark energy model with generalized uncertainty principle
• SNEMO: Improved Empirical Models for Type Ia Supernovae
• Tsallis Agegraphic Dark Energy Model
• Consistency testing for invariance of the speed of light at different redshifts: the newest results from strong lensing and type Ia supernovae observations
• Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
• Electromagnetic dark energy
• A Dark Energy Model with Generalized Uncertainty Principle in the Emergent, Intermediate and Logamediate Scenarios of the Universe
• Interacting new agegraphic Phantom model of dark energy in non-flat universe