  In this paper we propose a stationary solution of Einstein's field equations
describing Reissner-Nordstrom black hole in dark energy background. It is to be
regarded as the Reissner-Nordstrom black hole is embedded into the dark energy
solution producing Reissner-Nordstrom-dark energy black hole. We find that the
space-time geometry of Reissner-Nordstrom-dark energy solution is Petrov type
$D$ in the classification of space-times. It is also shown that the embedded
space-time possesses an energy-momentum tensor of the electromagnetic field
interacting with the dark energy having negative pressure. We find the
energy-momentum tensor for dark energy violates the the strong energy condition
due to the negative pressure, whereas that of the electromagnetic field obeys
the strong energy condition. It is shown that the time-like vector field for an
observer in the Reissner-Nordstrom-dark energy space is expanding,
accelerating, shearing and non-rotating. We investigate the surface gravity of
the horizons for the embedded dark energy black hole. The characteristic
properties of relativistic dark energy based on the de Sitter solution is
discussed in an appendix.
