A trace of inflation in the local behavior of cosmological constant
  Assuming the existence of a cosmological constant depending on time, we study
the evolution of this field in a local region of spacetime. Solving the
standard equations of Einstein Relativity in the weak field approximation we
find two asymptotes in the behavior of the cosmological constant. Their meaning
is the existence of an inflationary era both in the far past and in the future.
A trace of the initial acceleration of the Universe can be found also in the
local behavior of cosmological constant.
