William Bower Taylor

Summary

William Bower Taylor Kinetic Theories of Gravitation… (1876)

Thus the conditions assumed in the mathematical theory of heat are satisfied by supposing μ to be very large and q [the excursion of the wave] to be very small ; and the fulfillment of these conditions accounts for the great energy of calorific repulsion. . . Hence atoms of very small size, acting upon each other by the intervention of waves of which the excursions are very small, mutually repel with a very great force ; and at the same time, as was shown in the Theory of Heat, the force varies very rapidly with the distance.
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