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G. W. Horndeski, J. Math. Phys. 17 (1976) 1980
1980
Earlier work this paper cites.
S. L. Shapiro and S. A. Teukolsky, Black holes, white dwarfs and neutron stars
1983
Earlier work this paper cites.
C. Charmousis, G. Niz, A. Padilla and P. M. Saffin, JHEP 0908, 070 (2009), arXiv:0905.2579; M. Li and Y. Pang, JHEP 0908, 015 (2009), arXiv:0905.2751; K. Koyama and F. Arroja, JHEP 1003, 061 (2010), arXiv:0910.1998
Original
1998
Earlier work this paper cites.
B. Z. Foster and T. Jacobson, Phys. Rev. D 73 (2006) 064015; M. L. Graesser, A. Jenkins and M. B. Wise, Phys. Lett. B 613 (2005) 5
2005
Earlier work this paper cites.
B. Z. Foster, Phys. Rev. D 73 (2006) 104012, arXiv:gr-qc/0602004; C. Eling, Phys. Rev. D 73 (2006) 084026
2006
Earlier work this paper cites.
D. Blas, O. Pujolas and S. Sibiryakov, JHEP 10 (2009) 029, arXiv:0906.3046 [hep-th]
Original
2009
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A. Nicolis, R. Rattazzi, E. Trincherini, Phys. Rev. D 79 (2009) 064036, arXiv:0811.2197 [hep-th]
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2009
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2015

Haghani, Zahra, Harko, Tiberiu, Sepangi, Hamid Reza et al.

We modify the scalar Einstein-aether theory by breaking the Lorentz invariance of a gravitational theory coupled to a Galileon type scalar field.

This is done by introducing a Lagrange multiplier term into the action, thus ensuring that the gradient of the scalar field is time-like, with unit norm.
The theory can also be considered as an extension to the mimetic dark matter theory, by adding some derivative self interactions to the action, which keeps the equation of motion at most second order in time derivatives.
The cosmological implications of the model are discussed in detail.

G. W. Horndeski, J. Math. Phys. 17 (1976) 1980
1980
Earlier work this paper cites.
S. L. Shapiro and S. A. Teukolsky, Black holes, white dwarfs and neutron stars
1983
Earlier work this paper cites.
C. Charmousis, G. Niz, A. Padilla and P. M. Saffin, JHEP 0908, 070 (2009), arXiv:0905.2579; M. Li and Y. Pang, JHEP 0908, 015 (2009), arXiv:0905.2751; K. Koyama and F. Arroja, JHEP 1003, 061 (2010), arXiv:0910.1998
Original
1998
Earlier work this paper cites.
B. Z. Foster and T. Jacobson, Phys. Rev. D 73 (2006) 064015; M. L. Graesser, A. Jenkins and M. B. Wise, Phys. Lett. B 613 (2005) 5
2005
Earlier work this paper cites.
B. Z. Foster, Phys. Rev. D 73 (2006) 104012, arXiv:gr-qc/0602004; C. Eling, Phys. Rev. D 73 (2006) 084026
2006
Earlier work this paper cites.
D. Blas, O. Pujolas and S. Sibiryakov, JHEP 10 (2009) 029, arXiv:0906.3046 [hep-th]
Original
2009
Earlier work this paper cites.
A. Nicolis, R. Rattazzi, E. Trincherini, Phys. Rev. D 79 (2009) 064036, arXiv:0811.2197 [hep-th]
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2009
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C. Deffayet, G. Esposito-Farese, A. Vikman, Phys. Rev. D 79 (2009) 084003, arXiv:0901.1314 [hep-th]
Original
2009
Cited alongside, same era.
C. Deffayet, S. Deser and G. Esposito-Farese, Phys. Rev. D 80 (2009) 064015
2009
Cited alongside, same era.
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Original
2010
Cited alongside, same era.
T. Jacobson and D. Mattingly, Phys. Rev. D 64 (2001) 024028 ; T. Jacobson and D. Mattingly, Phys. Rev. D 70 (2004) 024003 ; W. Donnelly and T. Jacobson, Phys. Rev. D 82 (2010) 064032 ; W. Donnelly and T. Jacobson Phys. Rev. D 82 (2010) 081501
2010
Cited alongside, same era.
T. Jacobson, Phys. Rev. D 81 (2010) 101502, arXiv:1001.4823 [hep-th]; T. Jacobson, arXiv:1310.5115[gr-qc]

T. P. Sotiriou, J. Phys. Conf. Ser. 283 (2011) 012034, arXiv:1010.3218 [hep-th]
Original
2011
Later among the works it cites.
C. Deffayet, X. Gao, D. A. Steer and G. Zahariade, Phys. Rev. D. 84 (2011) 064039, arXiv:1103.3260 [hep-th]; T. Kobayashi, M. Yamaguchi and J. Yokoyama, Prog. Theor. Phys. 126 (2011) 511, arXiv:1105.5723 [hep-th]
Original
2011
Later among the works it cites.
V. A. Kostelecky and N. Russell, Rev. Mod. Phys. 83 (2011) 11; S. Liberati, Class. Quant. Grav. 30 (2013) 133001
2013
Later among the works it cites.
A. Chamseddin and V. Mukhanov, JHEP 1311 (2013) 135
2013
Later among the works it cites.
T. Harko, F. S.N. Lobo, S. Nojiri, S. D. Odintsov, Phys. Rev. D 84 (2011) 024020; Z. Haghani, T. Harko, F. S. N. Lobo, H. R. Sepangi, S. Shahidi, Phys. Rev. D 88 (2013) 044023
2013