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HADRONIC MATHEMATICS, MECHANICS AND CHEMISTRY 413A possible candidate is given by superconductors, as studied in Chapter 8 withelectrons moving at the maximal causal speed V max = c o . These media canbe either opaque to light (because V max < c), or be transparent, in which casec max = V max because the speed of light is not the maximal causal speed, but anordinary local speed, thus being bounded by V max . In case the media are opaqueto light, b 4 = 1/n 4 preserves its meaning as a geometrization of the density withsignificant meaning, such as the fact that media of Type 3 are more dense thanthose of Type 2 (because c I,3 > c I,2 .GROUP II, TYPE 4: n s < n 4 , n 4 = 1, ˆβ < β, ˆγ > γ, c = co , V max 1, ˆβ < β, ˆγ > γ, c < co , V max
414 RUGGERO MARIA SANTILLIGROUP II, TYPE 6: n s < n 4 , n 4 < 1, ˆβ < β, ˆγ > γ, c > co , V max n 4 , n 4 = 1, ˆβ < β, ˆγ > γ, c = co , V max >c o , V max > c.This is the first of three inhomogeneous and anisotropic media of highden sitythat are of primary relevance for hadronic mechansics because representing thehyperdense media inside hadrons, stars, quasars and other internal astrophysicalproblems. All media of this group have V max > c o and V max > c. The first ofthese three media has the geometric significance that the speed of light is thesame as that in vacuum, c = c o .GROUP III, TYPE 8: n s > n 4 , n 4 > 1, ˆβ < β, ˆγ > γ, c < co , V max >c o , V max > c.This is a second type of inhomogeneous and anisotropic media of high densitythat is conceivable for extreme astrophysical conditions, such as those in theinterior of black holes, in which the maximal causal speed is expected to have nolimit, but the speed of light is expected to be much smaller than that in vacuum,assuming that light can even propagate in media of such extreme densities.GROUP III, TYPE 9: n s > n 4 , n 4 < 1, ˆβ < β, ˆγ > γ, c > co , V max >c o , V max > c, V max > c.These media are experimentally verified in the interior of heavy hadrons (Section6.1.7, 6.1.8, 6.1.9), in the interior of the fireball of the Bose-Einstein correlation(Section 6.1.10) and other hyperdense inhomogeneous and anisotropic media.As we shall see, these last media do indeed permit the prediction, quantitativedevelopment and industrial realization of basically ”new” clean energies, such asenergies originating from mechanism in the interior of the neutron, rather than ina nuclear structure. Due to their societal need, readers are alerted that technicalcriticisms are solicited, welcome and appreciated as part of a serious scientific
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