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Gravity on a Brane in Infinite-Volume Extra Space

Gia Dvali, Gregory Gabadadze

TL;DR

This work extends the Dvali-Gabadadze-Porrati framework to branes in infinite-volume extra dimensions with $D>5$, showing that an induced four-dimensional Ricci scalar on a delta-function brane yields Einstein gravity on the brane while the bulk remains infrared-transparent to zero-momentum gravitons. The authors derive the on-brane Newton potential $V(r)=\frac{1}{8\pi \overline M^2 r}$ and demonstrate that the graviton propagator on the brane retains the 4D Einstein tensor structure, with higher-dimensional effects suppressed except for $p^2=0$ modes that can couple to the bulk. They discuss the inverse (infrared) behavior of the bulk, the possibility of solving or softening the cosmological constant problem via bulk-brane dynamics, and implications for hierarchy stabilization through nonperturbative brane-induced scales and large bulk state multiplicities. The paper also analyzes the hierarchy problem and cosmological constant problem within this infinite-volume setup, outlining scenarios in which $M$ can be low yet $\ar M$ is large, and identifying key open questions about flat-brane uniqueness, stability, and realistic cosmologies. Overall, the work proposes a novel gravity-on-brane mechanism with potential implications for fundamental scales and low-energy effective gravity.

Abstract

We generalize the mechanism proposed in [hep-th/0005016] and show that a four-dimensional relativistic tensor theory of gravitation can be obtained on a delta-function brane in flat infinite-volume extra space. In particular, we demonstrate that the induced Ricci scalar gives rise to Einstein's gravity on a delta-function type brane if the number of space-time dimensions is bigger than five. The bulk space exhibits the phenomenon of infrared transparency. That is to say, the bulk can be probed by gravitons with vanishing four-dimensional momentum square, while it is unaccessible to higher modes. This provides an attractive framework for solving the cosmological constant problem.

Gravity on a Brane in Infinite-Volume Extra Space

TL;DR

This work extends the Dvali-Gabadadze-Porrati framework to branes in infinite-volume extra dimensions with , showing that an induced four-dimensional Ricci scalar on a delta-function brane yields Einstein gravity on the brane while the bulk remains infrared-transparent to zero-momentum gravitons. The authors derive the on-brane Newton potential and demonstrate that the graviton propagator on the brane retains the 4D Einstein tensor structure, with higher-dimensional effects suppressed except for modes that can couple to the bulk. They discuss the inverse (infrared) behavior of the bulk, the possibility of solving or softening the cosmological constant problem via bulk-brane dynamics, and implications for hierarchy stabilization through nonperturbative brane-induced scales and large bulk state multiplicities. The paper also analyzes the hierarchy problem and cosmological constant problem within this infinite-volume setup, outlining scenarios in which can be low yet is large, and identifying key open questions about flat-brane uniqueness, stability, and realistic cosmologies. Overall, the work proposes a novel gravity-on-brane mechanism with potential implications for fundamental scales and low-energy effective gravity.

Abstract

We generalize the mechanism proposed in [hep-th/0005016] and show that a four-dimensional relativistic tensor theory of gravitation can be obtained on a delta-function brane in flat infinite-volume extra space. In particular, we demonstrate that the induced Ricci scalar gives rise to Einstein's gravity on a delta-function type brane if the number of space-time dimensions is bigger than five. The bulk space exhibits the phenomenon of infrared transparency. That is to say, the bulk can be probed by gravitons with vanishing four-dimensional momentum square, while it is unaccessible to higher modes. This provides an attractive framework for solving the cosmological constant problem.

Paper Structure

This paper contains 9 sections, 65 equations, 1 figure.

Figures (1)

  • Figure 1: The one-loop diagram which generates the 4D Ricci scalar $\overline R$. Wave lines denote gravitons, solid lines denote massive scalars/fermions. Vertical short lines on scalar/fermion propagators indicate that they are massive.