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1961
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1963
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1972
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1984
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1995
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G. R. Dvali, G. Gabadadze and M. Porrati, Phys. Lett. B 485
2000
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2003
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M. A. Luty, M. Porrati and R. Rattazzi, JHEP 0309
2003
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J. M. Cline, S. Jeon and G. D. Moore, Phys. Rev. D 70
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P. Creminelli, A. Nicolis, M. Papucci and E. Trincherini, JHEP 0509
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2016

Theoretical Aspects of Cosmic Acceleration

Trodden, Mark

Understand

Efforts to understand and map the possible explanations for the late time acceleration of the universe have led to a broad range of suggestions, ranging from the cosmological constant and straightforward dark energy, to exotically coupled models, to infrared modifications of General Relativity.

If we are to uncover which, if any, of these approaches might provide a serious answer to the problem, it is crucial to understand the constraints that theoretical consistency places on the models, and on the regimes in which they make predictions.
In this talk, delivered as an invited plenary lecture at the Dark Side of the Universe conference in Kyoto, Japan, I briefly describe some modern attempts to carry out this program and some of the more interesting ideas that have emerged.
As an example, I use the Galileon model, discussing how the Vainshtein mechanism occurs, and how a number of these theoretical problems arise around such backgrounds.

Built on

M. Froissart, Phys. Rev. 123
1961
Earlier work this paper cites.
A. Martin, Phys. Rev. 129
1963
Earlier work this paper cites.
A. I. Vainshtein, Phys. Lett. B 39
1972
Earlier work this paper cites.
R. M. Wald, Chicago, Usa: Univ. Pr. ( 1984) 491p
1984
Earlier work this paper cites.
M. E. Peskin and D. V. Schroeder, Reading, USA: Addison-Wesley (1995) 842 p
1995
Earlier work this paper cites.
G. R. Dvali, G. Gabadadze and M. Porrati, Phys. Lett. B 485
2000
Earlier work this paper cites.
S. M. Carroll, M. Hoffman and M. Trodden, Phys. Rev. D 68
2003
Earlier work this paper cites.
M. A. Luty, M. Porrati and R. Rattazzi, JHEP 0309
2003
Earlier work this paper cites.
J. M. Cline, S. Jeon and G. D. Moore, Phys. Rev. D 70
2004
Earlier work this paper cites.
P. Creminelli, A. Nicolis, M. Papucci and E. Trincherini, JHEP 0509
2005
Earlier work this paper cites.