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New Cosmological Solutions in Massive Gravity · Around

2012

New Cosmological Solutions in Massive Gravity

Kobayashi, Tsutomu, Siino, Masaru, Yamaguchi, Masahide et al.

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We find new, simple cosmological solutions with flat, open, and closed spatial geometries, contrary to the previous wisdom that only the open model is allowed.

The metric and the St\"{u}ckelberg fields are given explicitly, showing nontrivial configurations of the St\"{u}ckelberg in the usual Friedmann-Lema\^{i}tre-Robertson-Walker coordinates.
The solutions exhibit self-acceleration, while being free from ghost instabilities.
Our solutions can accommodate inhomogeneous dust collapse represented by the Lema\^{i}tre-Tolman-Bondi metric as well.

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