pith:UT46KV6V
Induced-Gravity Palatini-Like Higgs Inflation in Supergravity Confronts ACT DR6
Supergravity model of induced-gravity Higgs inflation matches ACT DR6 while breaking B-L symmetry at 10^16 GeV scales.
arxiv:2602.05623 v3 · 2026-02-05 · hep-ph · astro-ph.CO · hep-th
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We formulate within Supergravity a model of induced-gravity inflation, excellently consistent with ACT DR6, inspired by the Palatini gravity. The inflaton belongs in the decomposition of a conjugate pair of Higgs superfields which lead to the spontaneous breaking of a U(1)B-L symmetry at a scale close to the range (0.102-5.85)x10^16 GeV.
The Kaehler potential contains a real shift-symmetric contribution together with separate holomorphic and antiholomorphic logarithmic terms whose argument is interpreted as the inflaton-Ricci scalar coupling; these terms are assumed to produce canonical normalization, subplanckian field values, and energy scales below the effective-theory cutoff.
A Palatini-inspired induced-gravity inflation model in supergravity fits ACT DR6 data while embedding into a B-L extended MSSM with split SUSY and leptogenesis.
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| First computed | 2026-05-26T01:02:31.988075Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
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Canonical record JSON
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