2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/190479The inflationary attractor properties of the canonical scalar field and Born-Infeld field are investigated in the Randall-Sundrum II scenario with a Gauss-Bonnet term in the bulk action. We find that the inflationary attractor property will always hold for both the canonical and Born-Infeld fields for any allowed non-negative Gauss-Bonnet coupling. We also briefly discuss the possibility of explaining the suppressed lower multiples and running scalar spectral index simultaneously in the scenario of Gauss-Bonnet brane inflation.7 pages, no figures. An error in the discussion of BI field corrected, conclusion correctedHigh Energy Physics - PhenomenologyAstrophysicsHigh Energy Physics - TheoryInflationary attractor in Gauss-Bonnet brane cosmologytext