Statefinder parameters for interacting dark energy

Winfried Zimdahl, Diego Pavón

Research output: Contribution to journalArticleResearchpeer-review

135 Citations (Scopus)


We argue that the recently introduced "statefinder parameters" (Sahni et al., JETP Lett. 77, 201 (2003)), that include the third derivative of the cosmic scale factor, are useful tools to characterize interacting quintessence models. We specify the statefinder parameters for two classes of models that solve, or at least alleviate, the coincidence problem.
Original languageEnglish
Pages (from-to)1483-1491
JournalGeneral Relativity and Gravitation
Issue number6
Publication statusPublished - 1 Jun 2004


  • Accelerated expansion
  • Cosmology
  • Statefinder parameters


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