We consider the generation of thick brane configurations in a pure geometric Weyl integrable 5D space time which constitutes a non-Riemannian generalization of Kaluza-Klein (KK) theory. In this framework, we show how 4D gravity can be localized on a scalar thick brane which does not necessarily respect reflection symmetry, generalizing in this way several previous models based on the Randall-Sundrum (RS) system and avoiding both, the restriction to orbifold geometries and the introduction of the branes in the action by hand. We first obtain a thick brane solution that preserves 4D Poincar'e invariance and breaks Z_2-symmetry along the extra dimension which, indeed, can be either compact or extended, and supplements brane solutions previously found by other authors. In the non-compact case, this field configuration represents a thick brane with positive energy density centered at y=c_2, whereas pairs of thick branes arise in the compact case. Remarkably, the Weylian scalar curvature is non-singular along the fifth dimension in the non-compact case, in contraposition to the RS thin brane system. We also recast the wave equations of the transverse traceless modes of the linear fluctuations of the classical background into a Schr"odinger's equation form with a volcano potential of finite bottom in both the compact and the extended cases. We solve Schr"odinger equation for the massless zero mode m^2=0 and obtain a single bound wave function which represents a stable 4D graviton. We also get a continuum gapless spectrum of KK states with m^2>0 that are suppressed at y=c_2 and turn asymptotically into plane waves.

6 pages in PRD format, 3 figures, we corrected signs in the field equations, the expressions for the scalar field and the self-interacting potential. Due to the fact that no changes are introduced in the warp factor, the physics of the system remains the same