Sneutrino Inflation with $\alpha$-attractors
  Sneutrino inflation employs the fermionic partners of the inflaton and
stabilizer field as right-handed neutrinos to realize the seesaw mechanism for
light neutrino masses. We show that one can improve the latest version of this
scenario and its consistency with the Planck data by embedding it in the theory
of cosmological $\alpha$-attractors.
