“Insert d”, page 4
d.4 d.1 Another modality of action of the matter.
d.2 Useful values of the angular movement.
d.3 Other features of the “action d”.
d.4 “Action d” and thermodynamic balances.
d.5 Effects of the “action d” on the Earth.
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Thermodynamics in different forms of energy.
.1 The first two laws of thermodynamics have been formulated above all in the study of “short range energies”, such as the mechanical, electrical, and chemical ones, and applied to them successfully.
.2 As for the two “long range energies” (gravitation, and “action d”), in my opinion, we have to be ready to face different thermodynamic laws, because of the following considerations.
Effects of gravitation.
.3 The gravitation force starts processes of agglomeration, concentration, convergence, and orderly disposition of the matter - as many have already pointed out.
.4 This way, it prepares also the successive favourable conditions for the production of many forms of energy.
The movement.
.5 The gravitation rules also the movements of the celestial bodies.
.6 Those movements, at their turn, would originate another long range energy, extremely rich in neguentropy, the “action d”, which, at given circumstances, would trigger “type 2 dissipative reactions”, in open structure molecules.
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With regard to masses external to the Earth.
.7 The aforesaid “type 2 dissipative reactions”, those which would be brought about by the “action d”, generated by the relative movement of masses external to the Earth (the Moon, the Sun), would allow a substantial decrease of entropy in many systems, without an apparent consumption of energy.
.8 Unless one finds that also the movement of the masses entails some form of consumption. A topic to be studied.
With regard to the surrounding matter.
.9 A different question arises in case the movement is executed with respect to the surrounding matter.
.10 Then, there is certainly a consumption of energy, when you get either the water (insert Q), or the grains (experiment A, page 2.7) in motion .
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