  Despite two decades of tremendous experimental and theoretical progress, the
riddle of the accelerated expansion of the Universe remains to be solved. On
the experimental side, our understanding of the possibilities and limitations
of the major dark energy probes has evolved; here we summarize the major probes
and their crucial challenges. On the theoretical side, the taxonomy of
explanations for the accelerated expansion rate is better understood, providing
clear guidance to the relevant observables. We argue that: i) improving
statistical precision and systematic control by taking more data, supporting
research efforts to address crucial challenges for each probe, using
complementary methods, and relying on cross-correlations is well motivated; ii)
blinding of analyses is difficult but ever more important; iii) studies of dark
energy and modified gravity are related; and iv) it is crucial that R&D for a
vibrant dark energy program in the 2030s be started now by supporting studies
and technical R&D that will allow embryonic proposals to mature. Understanding
dark energy, arguably the biggest unsolved mystery in both fundamental particle
physics and cosmology, will remain one of the focal points of cosmology in the
forthcoming decade.
