Cosmological model with energy transfer

Abstract

The observations of SNIa suggest that we live in the acceleration epoch when the densities of the cosmological constant term and matter are almost equal. This leads to the cosmic coincidence conundrum. As the explanation for this problem we propose the FRW model with dark matter and dark energy which interact each other exchanging energy. We show that the cubic correction to the Hubble law, measured by distant supernovae type Ia, probes this interaction. We demonstrate that influences between nonrelativistic matter and vacuum sectors are controlled by third and higher derivatives of the scale factor. As an example we consider flat decaying $\Lambda (t)$ FRW cosmologies. We point out the possibility of measure of the energy transfer by the cubic and higher corrections to Hubble's law. The statistical analysis of SNIa data is used as an evidence of energy transfer. We find that there were the transfer from the dark energy sector to the dark matter one without any assumption about physics governing this process. We confront this hypothesis about the transfer with SNIa observations and find that the transfer the phantom and matter sector is admissible for ${\Omega }_{\text{m},0}=0.27$. We also demonstrate that it is possible to differentiate between the energy transfer model and the variable coefficient equation of state model.

RevTeX4, 8 pages, 4 figure; new section on testing the transfer from SNIa

References in corpus (1)

• Late Universe expansion dominated by domain walls and dissipative dark matter

Cited by in corpus (55)

• Dynamics of dark energy
• Probing the Coupling between Dark Components of the Universe
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Cosmologies with Energy Exchange
• Interacting Holographic Phantom
• Interacting dark energy, holographic principle and coincidence problem
• Holographic tachyon model of dark energy
• Cosmological coincidence problem in interacting dark energy models
• Entropic cosmology for a generalized black-hole entropy
• Interacting generalized Chaplygin gas model in non-flat universe
• Statefinder diagnosis in a non-flat universe and the holographic model of dark energy
• Observational $H(z)$ Data and Cosmological Models
• The Cosmological Dynamics of Interacting Holographic Dark Energy Model
• Generalized Second Law of Thermodynamics in $f(T)$ Gravity with Entropy Corrections
• Interacting dark energy in $f(R)$ gravity
• Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
• Evolution of the universe in entropic cosmologies via different formulations
• Interacting polytropic gas model of phantom dark energy in non-flat universe
• Dynamics of interacting quintessence
• Constraints on coupling constant between dark energy and dark matter
• Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• The generalized second law of gravitational thermodynamics on the apparent and event horizons in FRW cosmology
• Non-adiabatic-like accelerated expansion of the late universe in entropic cosmology
• AIC, BIC, Bayesian evidence against the interacting dark energy model
• Interacting Energy Components and Observational $H(z)$ Data
• The generalized second law in irreversible thermodynamics for the interacting dark energy in a non-flat FRW universe enclosed by the apparent horizon
• New coupled quintessence cosmology
• On the resolution of cosmic coincidence problem and phantom crossing with triple interacting fluids
• Interaction between dark energy and dark matter: observational constraints from OHD, BAO, CMB and SNe Ia
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• Falsifying cosmological models based on a non-linear electrodynamics
• Interacting new generalized Chaplygin gas
• Dynamics of coupled phantom and tachyon fields
• Towards testing interacting cosmology by distant type Ia supernovae
• Reconstructing interacting new agegraphic polytropic gas model in non-flat FRW universe
• Dark energy interacting with two fluids
• Cosmological model of the interaction between dark matter and dark energy
• The generalized second law for the interacting generalized Chaplygin gas model
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Testing the interaction model with cosmological data and gamma-ray bursts
• Holographic interacting dark energy in the braneworld cosmology
• The Influence of Evolving Dark Energy on Cosmology
• Phase space analysis of the bouncing universe with stringy effects
• Cosmic acceleration from interaction of ordinary fluids
• Constraints on interacting dynamical dark energy and a new test for $\Lambda$CDM
• Non-flat universe and interacting dark energy model
• Cosmological Constraints on Entropic Cosmology with Matter Creation
• Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy
• Interacting warm dark matter
• A new way to test the WIMP dark matter models
• Interacting dark fluid in the universe bounded by event horizon : A non-equilibrium prescription
• Do Black Holes Produce Phantom Energy?
• Generic autonomous system approach to interacting dark energy models
• A Thousand Problems in Cosmology: Interaction in the Dark Sector
• Reservoir-assisted energy migration through multiple spin-domains