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Observational constraints on holographic tachyonic dark energy in interaction with dark matter

2009/12/31 by S. Micheletti, Sandro M. R. Micheletti · 2 citations
Physics and Astronomy · #Astrophysics #Baryon acoustic oscillations #Black Holes and Theoretical Physics #Context (archaeology) #Cosmic microwave background #Cosmological constant #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark fluid #Dark matter #Higgs boson #Higgs field #Hot dark matter #Lambda-CDM model #Particle physics #Physics #Quantum mechanics #Scalar field dark matter #Tachyon #Tachyonic field #Theoretical physics #gr-qc

paper · pdf · doi:10.1088/1475-7516/2010/05/009

published as JCAP 1005:009,2010 · 14 pages, 5 figures

openalex publication_date 2010/05/12 · arxiv created 2010/05/13 · arxiv updated 2010/05/25 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06

Abstract

We discuss an interacting tachyonic dark energy model in the context of the holographic principle. The potential of the holographic tachyon field in interaction with dark matter is constructed. The model results are compared with CMB shift parameter, baryonic acoustic oscilations, lookback time and the Constitution supernovae sample. The coupling constant of the model is compatible with zero, but dark energy is not given by a cosmological constant.

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