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We show that, in generic higher-order scalar-tensor theories which avoid the Ostrogradsky instability, the presence of a scalar field significantly modifies the propagation of matter perturbations, even in weakly curved backgrounds.
To the problem of nonvanishing gravitation mass
A. I. Vainshtein · 1972
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Second-order scalar-tensor field equations in a four-dimensional space
Gregory Walter Horndeski · 1974
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Brookhaven National Laboratory selected cryogenic data notebook
J.E. Jensen, Cryogenic Data Center, and Brookhaven National Laboratory · 1980
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Handbook of the Speed of Sound in Real Gases
A.J. Zuckerwar and G.S.K. Wong · 2002
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An introduction to the Vainshtein mechanism
Eugeny Babichev and Cédric Deffayet · 2013
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Breaking of Vainshtein screening in scalar-tensor theories beyond Horndeski
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Jeremy Sakstein · 2015
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Hydrogen Burning in Low Mass Stars Constrains Scalar-Tensor Theories of Gravity
Jeremy Sakstein · 2015
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Astrophysical Probes of the Vainshtein Mechanism: Stars and Galaxies
Kazuya Koyama and Jeremy Sakstein · 2015
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Modified gravity inside astrophysical bodies
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B. P. Abbott et al · 2017
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Hamiltonian vs stability and application to Horndeski theory
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David Langlois, Ryo Saito, Daisuke Yamauchi, and Karim Noui · 2018
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