Built on

C. Deffayet, S. Deser and G. Esposito-Farese, Phys. Rev. D 80
Original
1967
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A. I. Vainshtein, Phys. Lett. B 39
1972
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C. Charmousis, E. J. Copeland, A. Padilla and P. M. Saffin, arXiv:1106.2000 [hep-th]
Original
2000
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G. R. Dvali, G. Gabadadze and M. Porrati, Phys. Lett. B 485
2000
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C. Deffayet, Phys. Lett. B 502
2001
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C. Deffayet, G. R. Dvali, G. Gabadadze and A. I. Vainshtein, Phys. Rev. D 65
2002
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C. Deffayet, G. R. Dvali and G. Gabadadze, Phys. Rev. D 65
2002
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M. A. Luty, M. Porrati and R. Rattazzi, JHEP 0309
2003
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G. Gabadadze and A. Iglesias, Phys. Lett. B 639
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C. Deffayet, S. Deser and G. Esposito-Farese, Phys. Rev. D 82
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2011

The Paths of Gravity in Galileon Cosmology

Appleby, Stephen A., Linder, Eric V.

Understand

Galileon gravity offers a robust gravitational theory for explaining cosmic acceleration, having a rich phenomenology of testable behaviors.

We explore three classes of Galileon models -- standard uncoupled, and linearly or derivatively coupled to matter -- investigating the expansion history with particular attention to early time and late time attractors, as well as the linear perturbations.
From the relativistic and nonrelativistic Poisson equations we calculate the generalizations of the gravitational strength (Newton's constant), deriving its early and late time behavior.
By scanning through the parameters we derive distributions of the gravitational strength at various epochs and trace the paths of gravity in its evolution.

Built on

C. Deffayet, S. Deser and G. Esposito-Farese, Phys. Rev. D 80
Original
1967
Earlier work this paper cites.
A. I. Vainshtein, Phys. Lett. B 39
1972
Earlier work this paper cites.
C. Charmousis, E. J. Copeland, A. Padilla and P. M. Saffin, arXiv:1106.2000 [hep-th]
Original
2000
Earlier work this paper cites.
G. R. Dvali, G. Gabadadze and M. Porrati, Phys. Lett. B 485
2000
Earlier work this paper cites.
C. Deffayet, Phys. Lett. B 502
2001
Earlier work this paper cites.
C. Deffayet, G. R. Dvali, G. Gabadadze and A. I. Vainshtein, Phys. Rev. D 65
2002
Earlier work this paper cites.
C. Deffayet, G. R. Dvali and G. Gabadadze, Phys. Rev. D 65
2002
Earlier work this paper cites.
M. A. Luty, M. Porrati and R. Rattazzi, JHEP 0309
2003
Earlier work this paper cites.
G. Gabadadze and A. Iglesias, Phys. Lett. B 639
2006
Earlier work this paper cites.
C. Charmousis, R. Gregory, N. Kaloper and A. Padilla, JHEP 0610
2006
Earlier work this paper cites.
E. Babichev, V. Mukhanov and A. Vikman, JHEP 0802
Original
2008
Earlier work this paper cites.
A. Nicolis, R. Rattazzi and E. Trincherini, Phys. Rev. D 79
Original
2009
Earlier work this paper cites.
C. Deffayet, G. Esposito-Farese and A. Vikman, Phys. Rev. D 79
Original
2009
Earlier work this paper cites.
F. P. Silva and K. Koyama, Phys. Rev. D 80
Original
2009
Earlier work this paper cites.
N. Chow and J. Khoury, Phys. Rev. D 80
Original
2009
Earlier work this paper cites.
C. Deffayet, S. Deser and G. Esposito-Farese, Phys. Rev. D 82
Original
2010
Earlier work this paper cites.
A. De Felice and S. Tsujikawa, JCAP 1007
Original
2010
Earlier work this paper cites.
A. De Felice, S. Mukohyama and S. Tsujikawa, Phys. Rev. D 82
Original
2010
Earlier work this paper cites.