Field theory model for dark matter and dark energy in interaction

Sandro Micheletti, Elcio Abdalla, and Bin Wang
Phys. Rev. D 79, 123506 – Published 15 June 2009

Abstract

We propose a field theory model for dark energy and dark matter in interaction. Comparing the classical solutions of the field equations with the observations of the CMB shift parameter, baryonic acoustic oscillations, lookback time, and the Gold supernovae sample, we observe a possible interaction between dark sectors with energy decay from dark energy into dark matter. The observed interaction provides an alleviation to the coincidence problem.

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  • Received 17 February 2009

DOI:https://doi.org/10.1103/PhysRevD.79.123506

©2009 American Physical Society

Authors & Affiliations

Sandro Micheletti1,*, Elcio Abdalla1,†, and Bin Wang2,‡

  • 1Instituto de Física, Universidade de São Paulo, CP 66318, 05315-970, São Paulo, Brazil
  • 2Department of Physics, Fudan University, 200433 Shanghai, China

  • *smrm@fma.if.usp.br
  • eabdalla@fma.if.usp.br
  • wangb@fudan.edu.cn

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Issue

Vol. 79, Iss. 12 — 15 June 2009

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