The evolution of a closed Friedmann universe filled by a tachyon scalar field with a trigonometric potential and cold dark matter (CDM) is investigated. A subset of the evolutions consistent to 1σ confidence level with the Union 2.1 supernova data set is identified. The evolutions of the tachyon field are classified. Some of them evolve into a de Sitter attractor, while others proceed through a pseudo-tachyonic regime into a sudden future singularity. Critical evolutions leading to Big Brake singularities in the presence of CDM are found and a new type of cosmological evolution characterized by singularity avoidance in the pseudo-tachyon regime is presented
In this work a tachyonization of the ΛCDM model for a spatially flat Friedmann-Robertson-Walker spac...
We investigate various dark energy models by taking into account the thermal effects induced from Ha...
Current observational evidence does not yet exclude the possibility that dark energy could be in the...
The evolution of a closed Friedmann universe filled by a tachyon scalar field with a trigonometric p...
A recently investigated tachyonic scalar field dark energy dominated universe exhibits a bivalent f...
We investigate a Friedmann universe filled with a tachyon scalar field, which behaves as dustlike ma...
We investigate a Friedmann universe filled with a tachyon scalar field, which behaved as dustlike ma...
We investigate the case of a homogeneous tachyon field coupled to gravity in a spatially flat Friedm...
We compare the existing observational data on type Ia supernovae with the evolutions of the Universe...
We investigate whether a tachyonic scalar field, encompassing both dark energy and dark matter-like...
We present a detailed study of cosmological effects of homogeneous tachyon matter coexisting with no...
We compare the existing observational data on type Ia supernovae with the evolutions of the Universe...
We study the role that tachyon fields may play in cosmology as compared to the well-established use ...
We examine an interacting dark matter variable vacuum energy model for a spatially flat Friedmann-Ro...
We study the evolving universe in the presence of dark energy via di®erent well-known cosmological ...
In this work a tachyonization of the ΛCDM model for a spatially flat Friedmann-Robertson-Walker spac...
We investigate various dark energy models by taking into account the thermal effects induced from Ha...
Current observational evidence does not yet exclude the possibility that dark energy could be in the...
The evolution of a closed Friedmann universe filled by a tachyon scalar field with a trigonometric p...
A recently investigated tachyonic scalar field dark energy dominated universe exhibits a bivalent f...
We investigate a Friedmann universe filled with a tachyon scalar field, which behaves as dustlike ma...
We investigate a Friedmann universe filled with a tachyon scalar field, which behaved as dustlike ma...
We investigate the case of a homogeneous tachyon field coupled to gravity in a spatially flat Friedm...
We compare the existing observational data on type Ia supernovae with the evolutions of the Universe...
We investigate whether a tachyonic scalar field, encompassing both dark energy and dark matter-like...
We present a detailed study of cosmological effects of homogeneous tachyon matter coexisting with no...
We compare the existing observational data on type Ia supernovae with the evolutions of the Universe...
We study the role that tachyon fields may play in cosmology as compared to the well-established use ...
We examine an interacting dark matter variable vacuum energy model for a spatially flat Friedmann-Ro...
We study the evolving universe in the presence of dark energy via di®erent well-known cosmological ...
In this work a tachyonization of the ΛCDM model for a spatially flat Friedmann-Robertson-Walker spac...
We investigate various dark energy models by taking into account the thermal effects induced from Ha...
Current observational evidence does not yet exclude the possibility that dark energy could be in the...