3.9 Article

Particle Production in an Expanding Universe Dominated by Dark Energy Fluid

Journal

GRAVITATION & COSMOLOGY
Volume 14, Issue 2, Pages 140-146

Publisher

MAIK NAUKA/INTERPERIODICA/SPRINGER
DOI: 10.1134/S0202289308020035

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Funding

  1. CNPq (Brazil)
  2. French/Brazilian scientific cooperation CAPES/COFECUB [506/05]

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We investigate particle production in an expanding universe dominated by a perfect fluid with the equation of state p = alpha rho. The rate of particle production, using the Bogoliubov coefficients, is determined exactly for any value of a in the case of alpha flat universe. When the strong energy condition is satisfied, the particle production rate decreases with time; the opposite occurs when the strong energy condition is violated. In the phantom case, the particle production rate diverges in a finite time for each mode represented by a wavenumber k. Nevertheless, the energy density associated with the produced particles tends to zero as the big rip is approached.

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