Constraints on Dark Energy from Inflation and the Swampland Conjectures
  We discuss the prospects of measuring deviations of the dark energy equation
of state from w=-1 by using the swampland conjectures to relate inflationary
models to quintessence scenarios. This note is based on work done by the author
with H. Murayama and C. Chiang arXiv:1811.01987.
