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University of Oslo & Caltech
Four-dimensional General Relativity from higher-dimensional Gauss-Bonnet gravity Ingunn Kathrine Wehus University of Oslo & Caltech Cosmo08, Madison August 26th, 2008 Based on Carroll and Wehus 2008, in preparation
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Four-dimensional General Relativity from higher-dimensional Gauss-Bonnet gravity
Natural generalization of GR in higher dimensions Special case of Lovelock gravity Compactification of the extra dimensions Give GR coupled to a scalar field in 4 dimensions Scalar field may be stabilized Gives pure GR, but with modified Planck mass May be relevant to the hierarchy problem
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Gauss-Bonnet The Gauss-Bonnet theorem in differential geometry connects the geometry (curvature) of a surface to its topology (Euler characteristic) In 2 dimensions the Ricci scalar R is a topological invariant. The action gives trivial field equations. However, in higher dimensions (D > 2) the same Lagrangian gives GR Similarily, in 4 dimensions the Gauss-Bonnet scalar B is a topological invariant The action gives trivial field equations for D=4. For D > 4 it gives Gauss-Bonnet gravity.
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Lovelock gravity In D = 2n (+1 if odd) dimensions the most general action yielding second order field equations for a dynamical spacetime metric is given by the Lovelock Lagrangian For example, the lowest order cases are
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Gauss-Bonnet gravity The combined GR and Gauss-Bonnet action in D dimensions, gives the equations of motion where For a maximally symmetric spacetime this simplifies to For D > 4, there are two vacuum solutions, and
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Compactification We now Kaluza-Klein compactify the extra dimensions, to obtain an effective theory for our ordinary four dimensional spacetime We then find
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Dimensional Reduction
Putting the previous expressions into the action and integrating over the extra dimensions gives where
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From Jordan frame to Einstein frame
The Weyl transformation, brings us to Einstein frame, where
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Stabilization by matter
Can various forms of matter help stabilize the scalar field? Some available components: Cosmological constant Magnetic field wrapped around extra dimensions Scalar fields Casimir energy due to the compact space Adding all these, one obtains the combined potential
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Pure Gauss-Bonnet We first consider the special case of pure Gauss-Bonnet, which, after dimensional reduction, gives the following effective action In n = 2 extra dimensions, this action is already in Einstein frame
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Scales and hierarchies
Adding matter gives the following potential for the scalar field Choosing for instance For b stabilized, the field equations reduce to where
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Summary Gauss-Bonnet gravity is a natural extension of General Relativity when considering higher dimensions Higher-dimensional Gauss-Bonnet gravity compactified to four dimensions reduces to General Relativity, coupled to a scalar field The details of this scalar-tensor theory differ from the GR case After stabilizing the scalar field, the four dimensional theory of gravity is pure General Relativity, but with a modified Planck mass
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