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arxiv: 1711.11051 · v2 · pith:ZNYG5BBQnew · submitted 2017-11-29 · ✦ hep-th · astro-ph.CO· gr-qc· hep-ph

From R² Gravity to No-Scale Supergravity

classification ✦ hep-th astro-ph.COgr-qchep-ph
keywords gravityno-scalesupergravityahlerbosonicconformalconformallyconstruction
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We show that $R^2$ gravity coupled conformally to scalar fields is equivalent to the real bosonic sector of SU(N,1)/SU(N)$\times$U(1) no-scale supergravity, where the conformal factor can be identified with the K\"ahler potential, and we review the construction of Starobinsky-like models of inflation within this framework.

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  1. Reheating in No-Scale Models of Inflation

    hep-ph 2026-06 unverdicted novelty 4.0

    Generalized no-scale models with R=2/(3α) for α≠1 or non-minimal gauge couplings allow unsuppressed inflaton decays, producing calculable reheating temperatures and (n_s,r) predictions.