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arXiv:2511.05545·v2·High Energy Physics — Phenomenology

Symmetry-Protected -Attractor Hybrid Inflation in Supergravity and Constraints from ACT DR6 and DESI DR2

Swapnil Kumar Singh🇮🇳

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Abstract

We present a symmetry-protected supergravity effective realization of hybrid -attractor inflation with a sequestered Stückelberg uplift. The model contains four chiral multiplets, an inflaton modulus , a stabilizer field , and a pair of oppositely charged waterfall multiplets , together with a hidden Stückelberg sector that generates an approximately constant positive contribution to the scalar potential. Along the real inflationary trajectory, the F-term potential realizes the E-model plateau \[ U(\phi)=V_0\left(1-e^{-\sqrt{2/(3\alpha)}\,\phi}\right)^2 , \] while the sequestered uplift shifts the total energy density without directly modifying the tree-level inflaton slope. We derive the background evolution, the analytic -- relation, the waterfall stability condition, and the leading predictions for the scalar spectral index and tensor-to-scalar ratio. The model retains the characteristic red-tilted -attractor behavior, with and tensor amplitudes controlled primarily by the curvature parameter , while the uplift and the hybrid end point generate only subleading corrections at fixed . We also discuss the assumptions required for an effectively single-field trajectory, including the treatment of the light angular component of , and examine the sensitivity of the sequestered uplift to Planck-suppressed cross-couplings. The resulting construction provides a controlled supergravity embedding of hybrid -attractor inflation compatible with current CMB constraints, including Planck, ACT DR6, and DESI DR2, while remaining testable by future -mode searches such as LiteBIRD and CMB-S4.

Comments: 33 pages, 3 figures, 2 tables; Accepted for publication in the Physics of the Dark Universe

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