Alleviation of Cosmic Age Problem In Interacting Dark Energy Model

Abstract

We investigate the cosmic age problem associated with the old high-$z$ quasar APM 08279 + 5255 and the oldest globular cluster M 107, both being difficult to accommodate in $\Lambda$CDM model. By evaluating the age of the Universe in a model that has an extremely phantom like form of dark energy (DE), we show that simply introducing the dark energy alone does not remove the problem, and the interaction between dark matter (DM) and DE need to be taken into account. Next, as examples, we consider two interacting DE models. It is found that both these two interacting DE Models can predict a cosmic age much greater than that of $\Lambda$CDM model at any redshift, and thus substantially alleviate the cosmic age problem. Therefore, the interaction between DM and DE is the crucial factor required to make the predicted cosmic ages consistent with observations.

12 pages, 3 figures, 5 tables, to appear in PLB

References in corpus (52)

• 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
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• The Cosmological Constant and Dark Energy
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Cosmological parameters from SDSS and WMAP
• Cosmological Imprint of an Energy Component with General Equation of State
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• Cosmological Constant - the Weight of the Vacuum
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• The Cosmological Constant
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• The 3D power spectrum of galaxies from the SDSS
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
• Cosmological Results from High-z Supernovae
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• Cosmological Tracking Solutions
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Cosmological Constraints from the SDSS Luminous Red Galaxies
• Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
• Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
• Scrutinizing Exotic Cosmological Models Using ESSENCE Supernova Data Combined with Other Cosmological Probes
• The Hubble Constant: A Summary of the HST Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids
• LBDS 53W091: An Old red Galaxy at z=1.552
• Solving the Coincidence Problem: Tracking Oscillating Energy
• High-redshift objects and the generalized Chaplygin gas
• Discovery of an ionized Fe-K edge in the z=3.91 Broad Absorption Line Quasar APM 08279+5255 with XMM-Newton
• Age Problem in the Holographic Dark Energy Model
• Scalar-field-dominated cosmology with a transient accelerating phase
• Constraining the cosmic equation of state from old galaxies at high redshift
• New limits on ${\Omega }_{\Lambda }$ and ${\Omega }_M$ from old galaxies at high redshift
• The State Equation of the Yang-Mills field Dark Energy Models
• Lookback time as a test for brane cosmology
• An old quasar in a young dark energy-dominated universe?
• Age of High Redshift Objects - a Litmus Test for the Dark Energy Models
• The Existence of an Old Quasar at $z=3.91$ and its Implications for $\Lambda (t)$ Deflationary Cosmologies
• The Cosmological Constant Problems (Talk given at Dark Matter 2000, February, 2000)
• 2-loop Quantum Yang-Mills Condensate as Dark Energy
• Yang-Mills condensate dark energy coupled with matter and radiation
• The Age of the Universe
• Coincidence Problem in YM Field Dark Energy Model
• Power-law Parameterized Quintessence Model
• Constraining scalar-tensor quintessence by cosmic clocks
• Is Thick Brane Model Consistent with the Recent Observations?
• Age constraints on the Agegraphic Dark Energy Model
• Cepheids, Supernovae, Ho, and the Age of the Universe

Cited by in corpus (44)

• Dark Energy
• Holographic Dark Energy
• Holographic dark energy models: A comparison from the latest observational data
• Probing interaction and spatial curvature in the holographic dark energy model
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• Running coupling: Does the coupling between dark energy and dark matter change sign during the cosmological evolution?
• Constraining dark energy with gamma-ray bursts
• Interacting Holographic Viscous Dark Energy Model
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Revisit of cosmic age problem
• Fitting the Constitution SNIa Data with Redshift Binned Parameterization Method
• Interacting model of new agegraphic dark energy: observational constraints and age problem
• Cosmic age problem revisited in the holographic dark energy model
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• Statefinder hierarchy model for the Barrow holographic dark energy
• Probing cosmic opacity at high redshifts with gamma-ray bursts
• Exploring the Systematic Uncertainties of Type Ia Supernovae as Cosmological Probes
• Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
• Exploring the Latest Union2 SNIa Dataset by Using Model-Independent Parametrization Methods
• A comprehensive investigation on the slowing down of cosmic acceleration
• Cosmic age test in inhomogeneous cosmological models mimicking $\Lambda$CDM on the light cone
• 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
• Exploring the evolution of color-luminosity parameter $\beta$ and its effects on parameter estimation
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• Self-interacting holographic dark energy
• Diagnosing $\Lambda$HDE model with statefinder hierarchy and fractional growth parameter
• More Evidence for the Redshift Dependence of Color from the JLA Supernova Sample Using Redshift Tomography
• New Primordial-Magnetic-Field Limit from The Latest LIGO S5 data
• Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models
• Exploring the cosmological consequences of JLA supernova data with improved flux-averaging technique
• Comparing dark energy models with current observational data
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• A Dark Energy Model in Lyra Manifold
• Cosmological implications of different baryon acoustic oscillation data
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• The torsion cosmology in Kaluza-Klein theory
• Evolution of cosmological perturbations in the models with interacting dynamical dark energy
• Observational constraints on a Yang-Mills condensate dark energy model
• A closer look at the cosmological implications of the $\Lambda$HDE model
• Probing Cosmic Acceleration by Using Model-Independent Parametrizations and Three Kinds of Supernova Statistics Techniques
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• Exploring the Latest Pantheon SNIa Dataset by Using Three Kinds of Statistics Techniques