Built on

C. Burrage and D. Seery, “Revisiting fifth forces in the Galileon model,” JCAP
Original
1927
Earlier work this paper cites.
E. J. Copeland, M. Sami, and S. Tsujikawa, “Dynamics of dark energy,” Int.J.Mod.Phys
1936
Earlier work this paper cites.
C. Deffayet, S. Deser, and G. Esposito-Farese, “Generalized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress-tensors,” Phys.Rev
Original
1967
Earlier work this paper cites.
A. Vainshtein, “To the problem of nonvanishing gravitation mass,” Phys.Lett
1972
Earlier work this paper cites.
M. A. Luty, M. Porrati, and R. Rattazzi, “Strong interactions and stability in the DGP model,” JHEP
2003
Earlier work this paper cites.
J. Khoury and A. Weltman, “Chameleon fields: Awaiting surprises for tests of gravity in space,” Phys.Rev.Lett
2004
Earlier work this paper cites.
A. Nicolis and R. Rattazzi, “Classical and quantum consistency of the DGP model,” JHEP
2004
Earlier work this paper cites.
S. Bharadwaj, S. P. Bhavsar, and J. V. Sheth, “The Size of the longest filaments in the universe,” Astrophys.J
2004
Earlier work this paper cites.
M. Pietroni, “Dark energy condensation,” Phys.Rev
2005
Earlier work this paper cites.

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2014

The Shape Dependence of Vainshtein Screening

Bloomfield, Jolyon K., Burrage, Clare, Davis, Anne-Christine

Understand

Scalar field theories that possess a Vainshtein mechanism are able to dynamically suppress the associated fifth forces in the presence of massive sources through derivative non-linearities.

The resulting equations of motion for the scalar are highly non-linear and therefore very few analytic solutions are known.
Here we present a brief investigation of the structure of Vainshtein screening in symmetrical configurations, focusing in particular on the spherical, cylindrical and planar solutions that are relevant for observations of the cosmic web.
We consider Vainshtein screening in both the Galileon model, where the non-linear terms involve second derivatives of the scalar, and a k-essence theory, where the non-linear terms involve only first derivatives of the scalar.

Built on

C. Burrage and D. Seery, “Revisiting fifth forces in the Galileon model,” JCAP
Original
1927
Earlier work this paper cites.
E. J. Copeland, M. Sami, and S. Tsujikawa, “Dynamics of dark energy,” Int.J.Mod.Phys
1936
Earlier work this paper cites.
C. Deffayet, S. Deser, and G. Esposito-Farese, “Generalized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress-tensors,” Phys.Rev
Original
1967
Earlier work this paper cites.
A. Vainshtein, “To the problem of nonvanishing gravitation mass,” Phys.Lett
1972
Earlier work this paper cites.
M. A. Luty, M. Porrati, and R. Rattazzi, “Strong interactions and stability in the DGP model,” JHEP
2003
Earlier work this paper cites.
J. Khoury and A. Weltman, “Chameleon fields: Awaiting surprises for tests of gravity in space,” Phys.Rev.Lett
2004
Earlier work this paper cites.
A. Nicolis and R. Rattazzi, “Classical and quantum consistency of the DGP model,” JHEP
2004
Earlier work this paper cites.
S. Bharadwaj, S. P. Bhavsar, and J. V. Sheth, “The Size of the longest filaments in the universe,” Astrophys.J
2004
Earlier work this paper cites.
M. Pietroni, “Dark energy condensation,” Phys.Rev
2005
Earlier work this paper cites.