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Possible Influence of Dark Energy on the Dark Matter Relic Abundance

  • Antonio Masiero
  • Francesca Rosati
Conference paper

Summary

Although a direct interaction between WIMP CDM candidates and scalar Quintessence fields (sources of Dark Energy) poses severe phenomenological threats, yet it is possible that the presence of Quintessence produces profound deviations in the expansion rate of the early Universe at the moment of WIMP decoupling, hence causing significant enhancements of the relic DM abundance. We consider the occurrence of such a phenomenon in a couple of physically interesting situations, kination and scalar-tensor theories of gravity where the scalar component plays the role of Quintessence. The consequences for supersymmetric DM candidates are briefly discussed.

Keywords

Dark Matter Dark Energy Hubble Parameter Expansion Rate Dark Matter Particle 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2006

Authors and Affiliations

  • Antonio Masiero
    • 1
  • Francesca Rosati
    • 1
  1. 1.Dipartimento di Fisica “Galileo Galilei” and INFN - Sezione di PadovaUniversità di PadovaPadovaItaly

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