2008/09/30 by Luis P. Chimento, Mónica Forte, Gilberto M. Kremer +1 · 6 citations
Physics and Astronomy · #Astrophysics #Black Holes and Theoretical Physics #Cosmological model #Cosmology #Cosmology and Gravitation Theories #Dark energy #Differential geometry #Geometry #Mathematical physics #Particle physics theoretical and experimental studies #Physics #Quintessence #Theoretical physics #gr-qc
paper · pdf · doi:10.1007/s10714-009-0924-5
published in General Relativity and Gravitation 42(6), 1523-1535 (Springer Science+Business Media) · Version accepted for publication in GRG
arxiv created 2009/12/18 · openalex publication_date 2010/01/20 · arxiv updated 2010/11/19 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In this work a tachyonization of the ΛCDM model for a spatially flat Friedmann-Robertson-Walker space-time is proposed. A tachyon field and a cosmological constant are considered as the sources of the gravitational field. Starting from a stability analysis and from the exact solutions for a standard tachyon field driven by a given potential, the search for a large set of cosmological models which contain the ΛCDM model is investigated. By the use of internal transformations two new kinds of tachyon fields are derived from the standard tachyon field, namely, a complementary and a phantom tachyon fields. Numerical solutions for the three kinds of tachyon fields are determined and it is shown that the standard and complementary tachyon fields reproduces the ΛCDM model as a limiting case. The standard tachyon field can also describe a transition from an accelerated to a decelerated regime, behaving as an inflaton field at early times and as a matter field at late times. The complementary tachyon field always behaves as a matter field. The phantom tachyon field is characterized by a rapid expansion where its energy density increases with time.