On the stability of renormalizable expansions in three-dimensional gravity

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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32 pages. (A further discussion to avoid tachyons is included. To be Published in Physical Review D.)

Scientific paper

10.1103/PhysRevD.50.7351

Preliminary investigations are made for the stability of the $1/N$ expansion in three-dimensional gravity coupled to various matter fields, which are power-counting renormalizable. For unitary matters, a tachyonic pole appears in the spin-2 part of the leading graviton propagator, which implies the unstable flat space-time, unless the higher-derivative terms are introduced. As another possibility to avoid this spin-2 tachyon, we propose Einstein gravity coupled to non-unitary matters. It turns out that a tachyon appears in the spin-0 or -1 part for any linear gauges in this case, but it can be removed if non-minimally coupled scalars are included. We suggest an interesting model which may be stable and possess an ultraviolet fixed point.

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