Built on

F. W. Hehl, P. Von Der Heyde, G. D. Kerlick and J. M. Nester, General Relativity with Spin and Torsion: Foundations and Prospects, Rev. Mod. Phys. 48 (1976) 393-416
1976
Earlier work this paper cites.
K. Hayashi and T. Shirafuji, New General Relativity, Phys. Rev. D 19 (1979) 3524
1979
Earlier work this paper cites.
B. L. Spokoiny, Inflation and Generation of Perturbations in Broken Symmetric Theory of Gravity, Phys. Lett. B 147 (1984) 39-43
1984
Earlier work this paper cites.
F. S. Accetta, D. J. Zoller and M. S. Turner, Induced Gravity Inflation, Phys. Rev. D 31 (1985) 3046
1985
Earlier work this paper cites.
T. Futamase and K. Maeda, Chaotic Inflationary Scenario In Models Having Nonminimal Coupling With Curvature, Phys. Rev. D 39 (1989) 399
1989
Earlier work this paper cites.
U. Kasper, On The Cosmological Constant Problem And Inflation In The Framework Of Nonminimal Coupling, Nuovo Cim. B 103 (1989) 291
1989
Earlier work this paper cites.
L. Amendola, M. Litterio and F. Occhionero, The Phase space view of inflation. 1: The nonminimally coupled scalar field, Int. J. Mod. Phys. A 5 (1990) 3861
1990
Earlier work this paper cites.
P. J. Steinhardt and F. S. Accetta, Hyperextended Inflation, Phys. Rev. Lett. 64 (1990) 2740
1990
Earlier work this paper cites.
A. O. Barvinsky and A. Y. Kamenshchik, Quantum scale of inflation and particle physics of the early universe, Phys. Lett. B 332 (1994) 270, gr-qc/9404062
1994
Earlier work this paper cites.
L. Amendola, Scaling solutions in general nonminimal coupling theories, Phys. Rev. D 60 (1999) 043501, astro-ph/9904120
1999
Earlier work this paper cites.
F. Perrotta, C. Baccigalupi and S. Matarrese, Extended quintessence, Phys. Rev. D 61 (2000) 023507, astro-ph/9906066
2000
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V. Sahni and S. Habib, Does inflationary particle production suggest Ω m \Omega_{m} less than 1 1 ?, Phys. Rev. Lett. 81 (1998) 1766, hep-ph/9808204; T. Chiba, Quintessence, the gravitational constant, and gravity, Phys. Rev. D60 (1999) 083508, gr-qc/9903094; J.P. Uzan, Cosmological scaling solutions of nonminimally coupled scalar fields, Phys. Rev. D 59 (1999) 123510, gr-qc/9903004; N. Bartolo and M. Pietroni, Scalar tensor gravity and quintessence, Phys. Rev. D 61 (2000) 023518, hep-ph/9908521; V. Faraoni, Inflation and quintessence with nonminimal coupling, Phys. Rev. D 62 (2000) 023504, gr-qc/0002091; E. Elizalde, S. Nojiri and S. D. Odintsov, Late-time cosmology in (phantom) scalar-tensor theory: Dark energy and the cosmic speed-up, Phys. Rev. D 70 (2004) 043539, hep-th/0405034
2000
Earlier work this paper cites.

Similar

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2000
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J. W. Maluf, J. Math. Phys. 35 (1994) 335; H. I. Arcos and J. G. Pereira, Int. J. Mod. Phys. D 13 (2004) 2193, gr-qc/0501017
2004
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Then

Shuang-Yong Zhou, A New Approach to Quintessence and Solution of Multiple Attractors, Phys. Lett. B 660 (2008) 7, arXiv:0705.1577 [astro-ph]; Wei Fang, Ying Li, Kai Zhang and Hui-Qing Lu, Exact Analysis of Scaling and Dominant Attractors Beyond the Exponential Potential, Class. Quant. Grav. 26 (2009) 155005, arXiv:0810.4193 [hep-th]
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L. Amendola, Cosmology with nonminimal derivative couplings, Phys. Lett. B 301 (1993) 175, gr-qc/9302010; S. F. Daniel and R. R. Caldwell, Consequences of a cosmic scalar with kinetic coupling to curvature, Class. Quant. Grav. 24 (2007) 5573, arXiv:0709.0009; E. N. Saridakis and S. V. Sushkov, Quintessence and phantom cosmology with non-minimal derivative coupling, Phys. Rev. D 81 (2010) 083510, arXiv:1002.3478 [gr-qc]; C. Germani and A. Kehagias, New Model of Inflation with Non-minimal Derivative Coupling of Standard Model Higgs Boson to Gravity, Phys. Rev. Lett. 105 (2010) 011302, arXiv:1003.2635 [hep-ph]

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2013

Scaling attractors in interacting teleparallel dark energy

Otalora, G.

Understand

It has been proposed recently the existence of a non-minimal coupling between a canonical scalar field (quintessence) and gravity in the framework of teleparallel gravity, motivated by similar constructions in the context of General Relativity.

The dynamics of the model, known as teleparallel dark energy, has been further developed, but no scaling attractor has been found.
Here we consider a model in which the non-minimal coupling is ruled by a dynamically changing coefficient $\alpha\equiv f_{,\phi}/\sqrt{f}$, with $f(\phi)$ an arbitrary function of the scalar field $\phi$.
It is shown that in this case the existence of scaling attractors is possible, which means that the universe will eventually enter these scaling attractors, regardless of the initial conditions.

Built on

F. W. Hehl, P. Von Der Heyde, G. D. Kerlick and J. M. Nester, General Relativity with Spin and Torsion: Foundations and Prospects, Rev. Mod. Phys. 48 (1976) 393-416
1976
Earlier work this paper cites.
K. Hayashi and T. Shirafuji, New General Relativity, Phys. Rev. D 19 (1979) 3524
1979
Earlier work this paper cites.
B. L. Spokoiny, Inflation and Generation of Perturbations in Broken Symmetric Theory of Gravity, Phys. Lett. B 147 (1984) 39-43
1984
Earlier work this paper cites.
F. S. Accetta, D. J. Zoller and M. S. Turner, Induced Gravity Inflation, Phys. Rev. D 31 (1985) 3046
1985
Earlier work this paper cites.
T. Futamase and K. Maeda, Chaotic Inflationary Scenario In Models Having Nonminimal Coupling With Curvature, Phys. Rev. D 39 (1989) 399
1989
Earlier work this paper cites.
U. Kasper, On The Cosmological Constant Problem And Inflation In The Framework Of Nonminimal Coupling, Nuovo Cim. B 103 (1989) 291
1989
Earlier work this paper cites.
L. Amendola, M. Litterio and F. Occhionero, The Phase space view of inflation. 1: The nonminimally coupled scalar field, Int. J. Mod. Phys. A 5 (1990) 3861
1990
Earlier work this paper cites.
P. J. Steinhardt and F. S. Accetta, Hyperextended Inflation, Phys. Rev. Lett. 64 (1990) 2740
1990
Earlier work this paper cites.
A. O. Barvinsky and A. Y. Kamenshchik, Quantum scale of inflation and particle physics of the early universe, Phys. Lett. B 332 (1994) 270, gr-qc/9404062
1994
Earlier work this paper cites.
L. Amendola, Scaling solutions in general nonminimal coupling theories, Phys. Rev. D 60 (1999) 043501, astro-ph/9904120
1999
Earlier work this paper cites.
F. Perrotta, C. Baccigalupi and S. Matarrese, Extended quintessence, Phys. Rev. D 61 (2000) 023507, astro-ph/9906066
2000
Earlier work this paper cites.
V. Sahni and S. Habib, Does inflationary particle production suggest Ω m \Omega_{m} less than 1 1 ?, Phys. Rev. Lett. 81 (1998) 1766, hep-ph/9808204; T. Chiba, Quintessence, the gravitational constant, and gravity, Phys. Rev. D60 (1999) 083508, gr-qc/9903094; J.P. Uzan, Cosmological scaling solutions of nonminimally coupled scalar fields, Phys. Rev. D 59 (1999) 123510, gr-qc/9903004; N. Bartolo and M. Pietroni, Scalar tensor gravity and quintessence, Phys. Rev. D 61 (2000) 023518, hep-ph/9908521; V. Faraoni, Inflation and quintessence with nonminimal coupling, Phys. Rev. D 62 (2000) 023504, gr-qc/0002091; E. Elizalde, S. Nojiri and S. D. Odintsov, Late-time cosmology in (phantom) scalar-tensor theory: Dark energy and the cosmic speed-up, Phys. Rev. D 70 (2004) 043539, hep-th/0405034
2000
Earlier work this paper cites.