Reheating in \(\alpha \)-attractors
\(\alpha \)-attractors is a very promising class of inflationary models, utilizing a non-canonical form of the kinetic term to solve the problem of flatness of the potential. This mechanism has significant implications for the dynamics of the (p)reheating. In the current manuscript, we extend past studies of the simple \(\alpha \)-attractor T-model (in linear approximation) to the recently proposed \(\alpha \)-attractor hypernatural T-model. Abstract Published by the Jagiellonian University 2025 authors
Authors
- Tomasz Krajewski (ORCID: https://orcid.org/0000-0002-1982-0944)
- M. Kulejewski (ORCID: https://orcid.org/0009-0004-5269-7003)
Publication Details
- Journal
- Acta Physica Polonica B Proceedings Supplement
- Published
- 2025-12-19
- DOI
- https://doi.org/10.5506/aphyspolbsupp.18.6-a4
- Primary Topic
- Cosmology and Gravitation Theories
- Type
- article
- Field-Weighted Citation Impact
- 0.00