Abstract
We show that R2 gravity coupled conformally to scalar fields is equivalent to the real bosonic sector of SU(N,1)/SU(N)×U(1) no-scale supergravity, where the conformal factor can be identified with the Kähler potential, and we review the construction of Starobinsky-like models of inflation within this framework.
Original language | English (US) |
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Article number | 043530 |
Journal | Physical Review D |
Volume | 97 |
Issue number | 4 |
DOIs | |
State | Published - Feb 26 2018 |
Bibliographical note
Publisher Copyright:© 2018 Published by the American Physical Society.