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A. E. Gumrukcuoglu, C. Lin and S. Mukohyama, arXiv:1206.2723 [hep-th]; M. S. Volkov, arXiv:1205.5713 [hep-th]; T. Kobayashi, M. Siino, M. Yamaguchi and D. Yoshida, arXiv:1205.4938 [hep-th]; D. Comelli, M. Crisostomi, F. Nesti and L. Pilo, arXiv:1204.1027 [hep-th]; N. Khosravi, H. R. Sepangi and S. Shahidi, arXiv:1202.2767 [gr-qc]; D. Comelli, M. Crisostomi, F. Nesti and L. Pilo, JHEP
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1983
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G. R. Dvali, G. Gabadadze and M. Porrati, Phys. Lett. B
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2013

Tasinato, Gianmassimo, Koyama, Kazuya, Niz, Gustavo

Massive gravity is a good theoretical laboratory to study modifications of General Relativity.

The theory offers a concrete set-up to study models of dark energy, since it admits cosmological self-accelerating solutions in the vacuum, in which the size of the acceleration depends on the graviton mass.
Moreover, non-linear gravitational self-interactions, in the proximity of a matter source, manage to mimic the predictions of linearised General Relativity, hence agreeing with solar-system precision measurements.
In this article, we review our work in the subject, classifying, on one hand, static solutions, and on the other hand, self-accelerating backgrounds.

M. Fierz, W. Pauli, Proc. Roy. Soc. Lond
1939
Earlier work this paper cites.
H. van Dam, M. J. G. Veltman, Nucl. Phys
1970
Earlier work this paper cites.
V. I. Zakharov, JETP Lett
1970
Earlier work this paper cites.
D. G. Boulware, S. Deser, Phys. Rev
1972
Earlier work this paper cites.
A. I. Vainshtein, Phys. Lett
1972
Earlier work this paper cites.
G.W. Horndeski, Int.J.Theor.Phys. 10 (1974)
1974
Earlier work this paper cites.
A. Salam and J. A. Strathdee, Phys. Rev. D
1977
Earlier work this paper cites.
A. E. Gumrukcuoglu, C. Lin and S. Mukohyama, arXiv:1206.2723 [hep-th]; M. S. Volkov, arXiv:1205.5713 [hep-th]; T. Kobayashi, M. Siino, M. Yamaguchi and D. Yoshida, arXiv:1205.4938 [hep-th]; D. Comelli, M. Crisostomi, F. Nesti and L. Pilo, arXiv:1204.1027 [hep-th]; N. Khosravi, H. R. Sepangi and S. Shahidi, arXiv:1202.2767 [gr-qc]; D. Comelli, M. Crisostomi, F. Nesti and L. Pilo, JHEP
Original
1983
Earlier work this paper cites.
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2000
Earlier work this paper cites.
C. Deffayet, Phys. Lett. B
2001
Earlier work this paper cites.
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2003
Earlier work this paper cites.

K. Koyama, Phys. Rev
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Cited alongside, same era.
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2005
Cited alongside, same era.
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2005
Cited alongside, same era.
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Original
2009
Cited alongside, same era.
C. de Rham and G. Gabadadze, Phys. Rev. D
Original
2010
Cited alongside, same era.
C. Deffayet, S. Deser and G. Esposito-Farese, Phys. Rev. D
Original
2010
Cited alongside, same era.