Cosmological dynamics of tachyonic teleparallel dark energy
Contribuinte(s) |
Universidade Estadual Paulista (UNESP) |
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Data(s) |
27/05/2014
27/05/2014
03/09/2013
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Resumo |
A detailed dynamical analysis of the tachyonic teleparallel dark energy model, in which a noncanonical scalar field (tachyon field) is nonminimally coupled to gravitation, is performed. It is found that, when the nonminimal coupling is ruled by a dynamically changing coefficient α≡f ,φ/√f, with f(φ) an arbitrary function of the scalar field φ, the Universe may experience a field-matter-dominated era φMDE, in which it has some portions of the energy density of φ in the matter dominated era. This is the most significant difference in relation to the so-called teleparallel dark energy scenario, in which a canonical scalar field (quintessence) is nonminimally coupled to gravitation. © 2013 American Physical Society. |
Identificador |
http://dx.doi.org/10.1103/PhysRevD.88.063505 Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 88, n. 6, 2013. 1550-7998 1550-2368 http://hdl.handle.net/11449/76503 10.1103/PhysRevD.88.063505 WOS:000323894000009 2-s2.0-84885011908 2-s2.0-84885011908.pdf |
Idioma(s) |
eng |
Relação |
Physical Review D: Particles, Fields, Gravitation and Cosmology |
Direitos |
closedAccess |
Tipo |
info:eu-repo/semantics/article |