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C. Deffayet, S. Deser, and G. Esposito-Farèse, Generalized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress-tensors, Phys. Rev. D80
Original
1967
Earlier work this paper cites.
J. B. Hartle, Slowly rotating relativistic stars. I. Equations of structure, Astrophys.J. 150
1967
Earlier work this paper cites.
J. B. Hartle and K. S. Thorne, Slowly Rotating Relativistic Stars. II. Models for Neutron Stars and Supermassive Stars, Astrophys.J. 153
1968
Earlier work this paper cites.
G. W. Horndeski, Second-order scalar-tensor field equations in a four-dimensional space, Int.J.Theor.Phys. 10
1974
Earlier work this paper cites.
T. Damour and G. Esposito-Farèse, Tensor-multi-scalar theories of gravitation, Class.Quant.Grav. 9
1992
Earlier work this paper cites.
T. Damour and G. Esposito-Farèse, Nonperturbative strong field effects in tensor - scalar theories of gravitation, Phys.Rev.Lett. 70
1993
Earlier work this paper cites.
M. Rainer and A. Zhuk, Tensor - multi - scalar theories from multidimensional cosmology, Phys. Rev. D54
1996
Earlier work this paper cites.
T. Damour and G. Esposito-Farèse, Tensor-scalar gravity and binary pulsar experiments, Phys.Rev. D54
1996
Earlier work this paper cites.
C. Armendariz-Picon, T. Damour, and V. F. Mukhanov, k-inflation, Phys. Lett. B458
1999
Earlier work this paper cites.
C. Charmousis, E. J. Copeland, A. Padilla, and P. M. Saffin, General second order scalar-tensor theory, self tuning, and the Fab Four, Phys. Rev. Lett. 108
Original
2000
Earlier work this paper cites.
G. T. Horowitz and V. E. Hubeny, Quasinormal modes of AdS black holes and the approach to thermal equilibrium, Phys. Rev. D62
2000
Earlier work this paper cites.
C. Armendariz-Picon, V. F. Mukhanov, and P. J. Steinhardt, Essentials of k-essence, Phys. Rev. D63
2001
Earlier work this paper cites.
M. Alishahiha, E. Silverstein, and D. Tong, DBI in the sky, Phys. Rev. D70
2004
Earlier work this paper cites.
D. Psaltis, Probes and Tests of Strong-Field Gravity with Observations in the Electromagnetic Spectrum, Living Rev. Rel. 11
Original
2008
Earlier work this paper cites.
P. Pani and V. Cardoso, Are black holes in alternative theories serious astrophysical candidates? The Case for Einstein-Dilaton-Gauss-Bonnet black holes, Phys.Rev. D79
Original
2009
Earlier work this paper cites.
C. Deffayet, S. Deser, and G. Esposito-Farese, Arbitrary p p -form Galileons, Phys. Rev. D82
Original
2010
Earlier work this paper cites.
T. Kobayashi, M. Yamaguchi, and J. Yokoyama, Generalized G-inflation: Inflation with the most general second-order field equations, Prog. Theor. Phys. 126
Original
2011
Earlier work this paper cites.
K. Van Acoleyen and J. Van Doorsselaere, Galileons from Lovelock actions, Phys. Rev. D83
Original
2011
Earlier work this paper cites.
C. de Rham and L. Heisenberg, Cosmology of the Galileon from Massive Gravity, Phys. Rev. D84
Original
2011
Earlier work this paper cites.
B. Kleihaus, J. Kunz, and E. Radu, Rotating Black Holes in Dilatonic Einstein-Gauss-Bonnet Theory, Phys. Rev. Lett. 106
Original
2011
Earlier work this paper cites.
P. Pani, E. Berti, V. Cardoso, and J. Read, Compact stars in alternative theories of gravity. Einstein-Dilaton-Gauss-Bonnet gravity, Phys.Rev. D84
Original
2011
Earlier work this paper cites.
T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Modified Gravity and Cosmology, Phys.Rept. 513
Original
2012
Earlier work this paper cites.
C. Germani, L. Martucci, and P. Moyassari, Introducing the Slotheon: a slow Galileon scalar field in curved space-time, Phys. Rev. D85
Original
2012
Earlier work this paper cites.
M. Rinaldi, Black holes with non-minimal derivative coupling, Phys. Rev. D86
Original
2012
Earlier work this paper cites.

Similar

T. Kolyvaris, G. Koutsoumbas, E. Papantonopoulos, and G. Siopsis, Scalar Hair from a Derivative Coupling of a Scalar Field to the Einstein Tensor, Class. Quant. Grav. 29
Original
2012
Cited alongside, same era.
T. Kobayashi, H. Motohashi, and T. Suyama, Black hole perturbation in the most general scalar-tensor theory with second-order field equations I: the odd-parity sector, Phys. Rev. D85
Original
2012
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K. Yagi, L. C. Stein, N. Yunes, and T. Tanaka, Post-Newtonian, Quasi-Circular Binary Inspirals in Quadratic Modified Gravity, Phys.Rev. D85
Original
2012
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P. C. Freire, N. Wex, G. Esposito-Farèse, J. P. Verbiest, M. Bailes, et al. , The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity, Mon. Not. Roy. Astron. Soc. 423
Original
2012
Cited alongside, same era.

Then

C. Bambi, Testing black hole candidates with electromagnetic radiation, (2015), arXiv:1509.03884 [gr-qc]
Original
2015
Later among the works it cites.
C. Charmousis, From Lovelock to Horndeski’s Generalized Scalar Tensor Theory, Proceedings of the 7th Aegean Summer School : Beyond Einstein’s theory of gravity. Modifications of Einstein’s Theory of Gravity at Large Distances. , Lect. Notes Phys. 892
Original
2015
Later among the works it cites.
M. Horbatsch, H. O. Silva, D. Gerosa, P. Pani, E. Berti, L. Gualtieri, and U. Sperhake, Tensor-multi-scalar theories: relativistic stars and 3 + 1 decomposition, Class. Quant. Grav. 32
Original
2015
Later among the works it cites.
S. Ohashi, N. Tanahashi, T. Kobayashi, and M. Yamaguchi, The most general second-order field equations of bi-scalar-tensor theory in four dimensions, JHEP 07
Original
2015
Later among the works it cites.

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2016

Compact objects in Horndeski gravity

Silva, Hector O., Maselli, Andrea, Minamitsuji, Masato et al.

Understand

Horndeski gravity holds a special position as the most general extension of Einstein's theory of general relativity with a single scalar degree of freedom and second-order field equations.

Because of these features, Horndeski gravity is an attractive phenomenological playground to investigate the consequences of modifications of general relativity in cosmology and astrophysics.
We present a review of the progress made so far in the study of compact objects (black holes and neutron stars) within Horndeski gravity.
In particular, we review our recent work on slowly rotating black holes and present some new results on slowly rotating neutron stars.