Cosmological coincidence problem in interactive dark energy models

Oct, 2006
13 pages
Published in:
  • Phys.Rev.D 74 (2006) 103007
e-Print:

Citations per year

20062011201620212025051015
Abstract: (arXiv)
An interacting dark energy model with interaction term Q=λmHρm+λdHρdQ= \lambda_m H\rho_m+\lambda_dH\rho_d is considered. By studying the model near the transition time, in which the system crosses the w=-1 phantom-divide-line, the conditions needed to overcome the coincidence problem is investigated. The phantom model, as a candidate for dark energy, is considered and for two specific examples, the quadratic and exponential phantom potentials, it is shown that it is possible the system crosses the w=-1 line, meanwhile the coincidence problem is alleviated, the two facts that have root in observations.
  • 95.36.+x
  • 98.80.Cq
  • 98.80.Jk
  • dark energy: interaction
  • phantom: potential
  • dark matter
  • equation of state
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