Inflation in Supergravity with a Single Chiral Superfield

Understand

We propose new supergravity models describing chaotic Linde- and Starobinsky-like inflation in terms of a single chiral superfield.

• The key ideas to obtain a positive vacuum energy during large field inflation are (i) stabilization of the real or imaginary partner of the inflaton by modifying a Kahler potential, and (ii) use of the crossing terms in the scalar potential originating from a polynomial superpotential.
• Our inflationary models are constructed by starting from the minimal Kahler potential with a shift symmetry, and are extended to the no-scale case.
• Our methods can be applied to more general inflationary models in supergravity with only one chiral superfield.