In physical cosmology, astronomy and celestial mechanics, dark
energy is a hypothetical form of energy that permeates all of space
and tends to increase the rate of expansion of the universe. Dark
energy is the most popular way to explain recent observations and
experiments that the universe appears to be expanding at an
accelerating rate. In the standard model of cosmology, dark energy
currently accounts for 74% of the total mass-energy of the
universe. This book presents and discusses the nature and
feasibility of laboratory registration using SQUID-magnetostrictor
systems; a review on dark energy objects; the dark energy scale in
superconductors; cosmic acceleration; a review of the quantum
Yang-Mills condensate (YMC) dark energy model; and others.
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