Fielding Hudson Garrison,
Popular Science Monthly
(1909)
“ By the second law (irreversible increase of entropy in natural processes) there is still greater probability that it tends to a final state of thermal equilibrium or death; and since the universe itself is so great, there is sufficient probability that other worlds than ours may deviate from thermal equilibrium. As a graphic exposition of this theory, which shows the vast scope of the second law of thermodynamics, a curve can be plotted with the variables H and the time as coordinates, to visualize what takes place in the universe. ”
