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Effective reheating in Gauss--Bonnet inflation with μ(ϕ,X) coupling

Ali Seidabadi, Sara Saghafi, Kourosh Nozari

astro-ph.COarXiv:2608.02506

Abstract

We study effective reheating in a scalar--Gauss--Bonnet inflationary model with a phase-space-dependent coupling μ(ϕ,X), in which a compact field-space feature is combined with a bounded kinetic gate. The modified inflationary background determines the pivot-scale quantities and the effective energy density at the end of inflation. These quantities are then used to derive the reheating duration N re and temperature T re through the thermal-history matching relation. We first perform two fixed-pivot reference scans by varying the overall Gauss--Bonnet strength λ GB and the kinetic parameter g_X separately. For the reference parameter choices, increasing either parameter increases N re and decreases T re for the selected reheating equations of state. Additional benchmark calculations clarify how these variations depend on the dynamical regime of the model. In the λ GB scan, the increase in N re and the decrease in T re persist, although both variations become strongly suppressed when the coupling is more localized or when the end of inflation is controlled more strongly by the E-model potential. In the g_X scan, stronger field-space localization and kinetic saturation can instead lead to a slight decrease in N re and an increase in T re as g_X is increased. When the bounded kinetic contribution is considered together with a weaker overall Gauss--Bonnet interaction, the resulting changes in the reheating quantities become nearly negligible. The fixed-pivot predictions of the representative and alternative benchmarks are compared with CMB constraints.These reheating constraints are then discussed for four representative values of the effective equation-of-state parameter, w re=-1/3,0,2/3, and 1.

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