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The Geometry of Doubly-Coupled Bigravity

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Cosmology Beyond Einstein

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Abstract

The existence of a consistent bimetric theory raises an intriguing question: which is the physical metric? In Chaps. 3 and 4 we chose to couple only one of the two metric, \(g_{\mu \textit{v}}\), directly to matter, while the other dynamical metric, \(f_{\mu \textit{v}}\), only interacts with matter fields indirectly through its interactions with \(g_{\mu \nu }\).

O, that way madness lies; let me shun that;

No more of that.

Lear, King Lear, 3.4

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Notes

  1. 1.

    Using the same principles, further candidate double couplings have been constructed in Ref. [11], but it is not yet known which, if any, of these are ghost-free.

  2. 2.

    Note that this is the \(\mathscr {O} (\epsilon )\) piece of Eq. (5.35). This form of the line element, \(f = p_\mu dx^\mu \), defines the Finsler one-form, \(p_\mu \) [17].

  3. 3.

    This will be the case in particular if \(g_{\mu \textit{v}}\) and \(f_{\mu \textit{v}}\) are conformally related, as then a lightlike path in one metric is also lightlike in the other.

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Correspondence to Adam Ross Solomon .

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Solomon, A.R. (2017). The Geometry of Doubly-Coupled Bigravity. In: Cosmology Beyond Einstein. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-46621-7_5

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