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Higher Derivative Quantum Gravity with Gauss-Bonnet Term

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arxiv hep-th/0412249 v2 pith:XSMUUHYY submitted 2004-12-21 hep-th

classification hep-th
keywords epsiloncasequantumtermapproachderivativeequationsgeneral
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

Higher derivative theory is one of the important models of quantum gravity, renormalizable and asymptotically free within the standard perturbative approach. We consider the $4-\epsilon$ renormalization group for this theory, an approach which proved fruitful in $2-\epsilon$ models. A consistent formulation in dimension $n=4-\epsilon$ requires taking quantum effects of the topological term into account, hence we perform calculation which is more general than the ones done before. In the special $n=4$ case we confirm a known result by Fradkin-Tseytlin and Avramidi-Barvinsky, while contributions from topological term do cancel. In the more general case of $4-\epsilon$ renormalization group equations there is an extensive ambiguity related to gauge-fixing dependence. As a result, physical interpretation of these equations is not universal unlike we treat $\epsilon$ as a small parameter. In the sector of essential couplings one can find a number of new fixed points, some of them have no analogs in the $n=4$ case.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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    A specific nonminimal kinetic term for the pure tensorial component of torsion makes the gravitational couplings of quadratic gravity asymptotically free at one loop while preserving the absence of tachyons.

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    Proper-time FRG applied to gravity-coupled O(N) scalars largely reproduces scaling solutions and critical properties found with the effective average action, with some quantitative differences at finite and large N de...

  3. Scalar model of effective field theory in curved space

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    In a two-scalar model, one-loop diagrams with mixed light and heavy internal lines collapse to local tadpole contributions in the infrared, matching the effective low-energy quartic theory in flat and weakly curved spacetime.

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