skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Non-minimally coupled tachyon field in teleparallel gravity

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2]
  1. Department of Physics, Babol Branch, Islamic Azad University, Shariati Street, Babol (Iran, Islamic Republic of)
  2. Department of Basic Sciences, Babol University of Technology, Shariati Street, Babol (Iran, Islamic Republic of)

We perform a full investigation on dynamics of a new dark energy model in which the four-derivative of a non-canonical scalar field (tachyon) is non-minimally coupled to the vector torsion. Our analysis is done in the framework of teleparallel equivalent of general relativity which is based on torsion instead of curvature. We show that in our model there exists a late-time scaling attractor (point P{sub 4}), corresponding to an accelerating universe with the property that dark energy and dark matter densities are of the same order. Such a point can help to alleviate the cosmological coincidence problem. Existence of this point is the most significant difference between our model and another model in which a canonical scalar field (quintessence) is used instead of tachyon field.

OSTI ID:
22525886
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2015, Issue 04; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

Scaling attractors in interacting teleparallel dark energy
Journal Article · Mon Jul 01 00:00:00 EDT 2013 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22525886

Dark energy cosmology with tachyon field in teleparallel gravity
Journal Article · Fri Jul 15 00:00:00 EDT 2016 · Journal of Experimental and Theoretical Physics · OSTI ID:22525886

Weyl-Cartan-Weitzenböck gravity as a generalization of teleparallel gravity
Journal Article · Mon Oct 01 00:00:00 EDT 2012 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22525886