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PreprintCC BY 4.0arXiv

Waterfall-modulated α-attractors

Abstract

Hybrid α-attractor models \cite{Kallosh:2022ggf} can have significantly greater values of ns and smaller r, while preserving the relation r≅ 3α(1−ns)2, which is valid for exponential T- and E-models at large values of the inflaton field. Here we study single-field α-attractors with features inspired by hybrid models: one can uplift the potential, and one can also have a waterfall regime that leads to a premature termination of inflation near the critical point φc. This allows one to increase the effective number of e-foldings Nc in formulas like ns≃ 1−2over Nc, r≃ 12 αover Nc2. By changing the waterfall's steepness and location, one can continuously move the predictions along the curves with r≅ 3α(1−ns)2 as ns increases and r decreases. We also study the effect of waterfall insertions and uplift on ns in quintessential α-attractors that describe inflation and dynamical dark energy.

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BibTeX
@misc{kallosh2026waterfallmodulated,
  title = {{Waterfall-modulated $α$-attractors}},
  author = {Renata Kallosh and Andrei Linde and Yusuke Yamada},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2608.12819},
  eprint = {2608.12819},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2608.12819},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Waterfall-modulated α-attractors
AU  - Renata Kallosh
AU  - Andrei Linde
AU  - Yusuke Yamada
PY  - 2026
DA  - 2026/09/01
PB  - arXiv
DO  - 10.48550/arxiv.2608.12819
UR  - https://arxiv.org/abs/2608.12819
AB  - Hybrid α-attractor models \cite{Kallosh:2022ggf} can have significantly greater values of n_s and smaller r, while preserving the relation r≅ 3α(1−n_s)^2, which is valid for exponential T- and E-models at large values of the inflaton field. Here we study single-field α-attractors with features inspired by hybrid models: one can uplift the potential, and one can also have a waterfall regime that leads to a premature termination of inflation near the critical point φ_c. This allows one to increase the effective number of e-foldings N_c in formulas like n_s≃ 1−2over N_c, r≃ 12 αover N_c^2. By changing the waterfall's steepness and location, one can continuously move the predictions along the curves with r≅ 3α(1−n_s)^2 as n_s increases and r decreases. We also study the effect of waterfall insertions and uplift on n_s in quintessential α-attractors that describe inflation and dynamical dark energy.
ER  -