Built on

E. J. Copeland, M. Sami, and S. Tsujikawa, Dynamics of dark energy
1936
Earlier work this paper cites.
S. Weinberg, Photons and gravitons in perturbation theory: Derivation of Maxwell’s and Einstein’s equations
1965
Earlier work this paper cites.
A. Vainshtein, To the problem of nonvanishing gravitation mass
1972
Earlier work this paper cites.
Supernova Search Team
1998
Earlier work this paper cites.
Supernova Cosmology Project
1999
Earlier work this paper cites.
B. Bertotti, L. Iess, and P. Tortora, A test of general relativity using radio links with the Cassini spacecraft
2003
Earlier work this paper cites.
J. Khoury and A. Weltman, Chameleon fields: Awaiting surprises for tests of gravity in space
2004
Earlier work this paper cites.
J. Khoury and A. Weltman, Chameleon cosmology
2004
Earlier work this paper cites.
P. Brax, C. van de Bruck, A.-C. Davis, J. Khoury, and A. Weltman, Detecting dark energy in orbit - The Cosmological chameleon
2004
Earlier work this paper cites.

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K. A. Olive and M. Pospelov, Environmental dependence of masses and coupling constants
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H. Oyaizu, M. Lima, and W. Hu, Nonlinear evolution of f(R) cosmologies. 2. Power spectrum
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Then

P. Brax and G. Pignol, Strongly Coupled Chameleons and the Neutronic Quantum Bouncer
Original
2011
Later among the works it cites.
T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Modified Gravity and Cosmology
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2012
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C. de Rham, G. Gabadadze, and A. J. Tolley, Ghost free Massive Gravity in the Stúckelberg language
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2012
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C. de Rham, Galileons in the Sky
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2012
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A. Upadhye, W. Hu, and J. Khoury, Quantum Stability of Chameleon Field Theories
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2012

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2012

Lectures on Screened Modified Gravity

Brax, Philippe

Understand

The acceleration of the expansion of the Universe has led to the construction of Dark Energy models where a light scalar field may have a range reaching up to cosmological scales.

Screening mechanisms allow these models to evade the tight gravitational tests in the solar system and the laboratory.
I will briefly review some of the salient features of screened modified gravity models of the chameleon, dilaton or symmetron types using $f(R)$ gravity as a template.

Built on

E. J. Copeland, M. Sami, and S. Tsujikawa, Dynamics of dark energy
1936
Earlier work this paper cites.
S. Weinberg, Photons and gravitons in perturbation theory: Derivation of Maxwell’s and Einstein’s equations
1965
Earlier work this paper cites.
A. Vainshtein, To the problem of nonvanishing gravitation mass
1972
Earlier work this paper cites.
Supernova Search Team
1998
Earlier work this paper cites.
Supernova Cosmology Project
1999
Earlier work this paper cites.
B. Bertotti, L. Iess, and P. Tortora, A test of general relativity using radio links with the Cassini spacecraft
2003
Earlier work this paper cites.
J. Khoury and A. Weltman, Chameleon fields: Awaiting surprises for tests of gravity in space
2004
Earlier work this paper cites.
J. Khoury and A. Weltman, Chameleon cosmology
2004
Earlier work this paper cites.
P. Brax, C. van de Bruck, A.-C. Davis, J. Khoury, and A. Weltman, Detecting dark energy in orbit - The Cosmological chameleon
2004
Earlier work this paper cites.