Warm Quintessential Inflation
  We introduce warm quintessential inflation and study it in the weak
dissipative regime. We consider the original quintessential inflation model,
which approximates quartic chaotic inflation at early times and thawing quartic
inverse-power-law quintessence at present. We find that the model successfully
accounts for both inflation and dark energy observations, while it naturally
reheats the Universe, thereby overcoming a major problem of quintessential
inflation model-building.
