Wall Solution with Weak Gravity Limit in Five Dimensional Supergravity
Masato Arai, Shigeo Fujita, Masashi Naganuma, Norisuke Sakai

TL;DR
This paper presents exact BPS wall solutions in five-dimensional supergravity, including a Randall-Sundrum-like model without fine-tuning, and explores various warp factor behaviors through potential deformations.
Contribution
It provides new exact solutions for BPS walls in five-dimensional supergravity with gravitational deformations of the Eguchi-Hanson model, including a Randall-Sundrum limit.
Findings
Warp factor decreases at both infinities in the thin wall limit.
Randall-Sundrum model obtained without fine-tuning.
Wall solutions with flat or increasing warp factors achieved by potential deformation.
Abstract
In five-dimensional supergravity, an exact solution of BPS wall is found for a gravitational deformation of the massive Eguchi-Hanson nonlinear sigma model. The warp factor decreases for both infinities of the extra dimension. Thin wall limit gives the Randall-Sundrum model without fine-tuning of input parameters. We also obtain wall solutions with warp factors which are flat or increasing in one side, by varying a deformation parameter of the potential.
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