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Anisotropy dissipation in brane-world inflation

Roy Maartens·Varun Sahni·Tarun Deep Saini
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Abstract

We examine the behavior of an anisotropic brane-world in the presence of inflationary scalar fields. We show that, contrary to naive expectations, a large anisotropy does not adversely affect inflation. On the contrary, a large initial anisotropy introduces more damping into the scalar field equation of motion, resulting in greater inflation. The rapid decay of anisotropy in the brane-world significantly increases the class of initial conditions from which the observed universe could have originated. This generalizes a similar result in general relativity. A unique feature of Bianchi I brane-world cosmology appears to be that for scalar fields with a large kinetic term the initial expansion of the universe is quasi-isotropic. The universe grows more anisotropic during an intermediate transient regime until anisotropy finally disappears during inflationary expansion.

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Roy Maartens, Varun Sahni, Tarun Deep Saini. 2001-02-06. Anisotropy dissipation in brane-world inflation. https://doi.org/10.1103/physrevd.63.063509

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