Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive gravity - INSPIRE

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Anisotropic Friedmann-Robertson-Walker universe from nonlinear massive gravity

A.Emir Gumrukcuoglu
(
- Tokyo U., IPMU
)
,
Chunshan Lin
(
- Tokyo U., IPMU
)
,
Shinji Mukohyama
(
- Tokyo U., IPMU
)

Jun, 2012

4 pages

Published in:

Phys.Lett.B 717 (2012) 295-298

Published: Oct 31, 2012

e-Print:

1206.2723 [hep-th]

DOI:

10.1016/j.physletb.2012.09.049

Report number:

IPMU12-0123

View in:

ADS Abstract Service

reference search121 citations

Citations per year

Abstract: (Elsevier)

Motivated by the recent no-go result of homogeneous and isotropic solutions in the nonlinear massive gravity, we study fixed points of evolution equations for a Bianchi type-I universe. We find a new attractor solution with non-vanishing anisotropy, on which the physical metric is isotropic but the Stückelberg configuration is anisotropic. As a result, at the background level, the solution describes a homogeneous and isotropic universe, while a statistical anisotropy is expected from perturbations, suppressed by smallness of the graviton mass.

Note:

4 pages, 1 figure, REVTeX4/ V2 with minor revison, and to appear on PLB

space-time: Robertson-Walker
anisotropy: statistical
gravitation: massive
gravitation: nonlinear
evolution equation
fixed point
attractor
space-time: Bianchi
cosmological model: anisotropy
Friedman model

References(25)

Figures(1)

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in preparation

A. de Felice
,
A.E. Gumrukcuoglu
,
C. Lin
,
S. Mukohyama