Built on

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2012

Linear perturbations in Galileon gravity models

Barreira, Alexandre, Li, Baojiu, Baugh, Carlton et al.

Understand

We study the cosmology of Galileon modified gravity models in the linear perturbation regime.

We derive the fully covariant and gauge invariant perturbed field equations using two different methods, which give consistent results, and solve them using a modified version of the {\tt CAMB} code.
We find that, in addition to modifying the background expansion history and therefore shifting the positions of the acoustic peaks in the cosmic microwave background (CMB) power spectrum, the Galileon field can cluster strongly from early times, and causes the Weyl gravitational potential to grow, rather than decay, at late times.
This leaves clear signatures in the low-$l$ CMB power spectrum through the modified integrated Sachs-Wolfe effect, strongly enhances the linear growth of matter density perturbations and makes distinctive predictions for other cosmological signals such as weak lensing and the power spectrum of density fluctuations.

Built on

C. Burrage and D. Seery, JCAP 1008
Original
1927
Earlier work this paper cites.
C. Deffayet, S. Deser, and G. Esposito-Farese, Phys.Rev. D80
Original
1967
Earlier work this paper cites.
A. Vainshtein, Phys. Lett. B 39
1972
Earlier work this paper cites.
G. W. Horndeski, Int.J.Theor.Phys. 10
1974
Earlier work this paper cites.
S. A. Appleby and E. V. Linder, JCAP 1203
Original
1981
Earlier work this paper cites.
T. Damour, G. W. Gibbons, and C. Gundlach, Phys. Rev. Lett. 64
1990
Earlier work this paper cites.
L. Amendola, Phys.Lett. B301
1993
Earlier work this paper cites.
C.-P. Ma and E. Bertschinger, Astrophys. J.(1994), arXiv:astro-ph/9401007 [astro-ph]
1994
Earlier work this paper cites.
S. Baeßler, B. R. Heckel, E. G. Adelberger, J. H. Gundlach, U. Schmidt, and H. E. Swanson, Phys. Rev. Lett. 83
1999
Earlier work this paper cites.
A. Challinor and A. Lasenby, Astrophys.J. 513
1999
Earlier work this paper cites.
G. Dvali, G. Gabadadze, and M. Porrati, Phys. Lett. B 485
2000
Earlier work this paper cites.
C. Charmousis, E. J. Copeland, A. Padilla, and P. M. Saffin, Phys.Rev.Lett. 108
Original
2000
Earlier work this paper cites.
D. J. Eisenstein, J. Annis, J. E. Gunn, A. S. Szalay, A. J. Connolly, R. C. Nichol, N. A. Bahcall, M. Bernardi, and et al., Ap J 122
2001
Earlier work this paper cites.
M. A. Luty, M. Porrati, and R. Rattazzi, JHEP 9
2003
Earlier work this paper cites.
M. A. Luty, M. Porrati, and R. Rattazzi, JHEP 2003
2003
Earlier work this paper cites.
A. Nicolis and R. Rattazzi, JHEP 6
2004
Earlier work this paper cites.
A. Nicolis and R. Rattazzi, JHEP 2004
2004
Earlier work this paper cites.
J. Khoury and A. Weltman, Phys. Rev. D 69
2004
Earlier work this paper cites.
P. Brax, C. van de Bruck, A.-C. Davis, J. Khoury, and A. Weltman, Phys. Rev. D 70
2004
Earlier work this paper cites.
S. M. Carroll, A. De Felice, V. Duvvuri, D. A. Easson, M. Trodden, et al. , Phys.Rev. D71
2005
Earlier work this paper cites.
E. J. Copeland, M. Sami, and S. Tsujikawa, Int. J. Mod. Phys. D 15
2006
Earlier work this paper cites.
D. Gorbunov, K. Koyama, and S. Sibiryakov, Phys. Rev. D 73
2006
Earlier work this paper cites.
A. Lewis and A. Challinor, Phys.Rept. 429
2006
Earlier work this paper cites.
R. P. Woodard, Lect.Notes Phys. 720
2007
Earlier work this paper cites.
G. V. Kulkarni, R. C. Nichol, R. K. Sheth, H.-J. Seo, D. J. Eisenstein, and A. Gray, MNRAS 378
2007
Earlier work this paper cites.
P. Brax, C. van de Bruck, A.-C. Davis, and D. J. Shaw, Phys.Rev. D78
Original
2008
Earlier work this paper cites.
R. E. Angulo, C. M. Baugh, C. S. Frenk, and C. G. Lacey, MNRAS 383
2008
Earlier work this paper cites.
D. A. Wake, R. K. Sheth, R. C. Nichol, C. M. Baugh, J. Bland-Hawthorn, M. Colless, W. J. Couch, S. M. Croom, R. de Propris, M. J. Drinkwater, A. C. Edge, J. Loveday, T. Y. Lam, K. A. Pimbblet, I. G. Roseboom, N. P. Ross, D. P. Schneider, T. Shanks, and R. G. Sharp, MNRAS 387
Original
2008
Earlier work this paper cites.
A. Nicolis, R. Rattazzi, and E. Trincherini, Phys. Rev. D 79
2009
Earlier work this paper cites.
C. Deffayet, G. Esposito-Farèse, and A. Vikman, Phys. Rev. D 79
2009
Earlier work this paper cites.
E. Babichev, C. Deffayet, and R. Ziour, Int.J.Mod.Phys. D18
Original
2009
Earlier work this paper cites.
N. Chow and J. Khoury, Phys. Rev. D 80
2009
Earlier work this paper cites.