hadronic mathematics, mechanics and chemistry - Institute for Basic ...

832 RUGGERO MARIA SANTILLIGROUP II, TYPE 5: n s < n 4 , n 4 > 1, ˆβ < β, ˆγ > γ, c < co , V max 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 high densitythat are of primary relevance for hadronic mechanics 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 noat large is sufficient to prohibit the exact validity of Einsteinian doctrines due to their strict isotropiccharacter, since anisotropy has deep geometric and dynamical implications. The appropriate broadeningof Einsteinian doctrines that is applicable for basic advances in the representation of anisotropic systems,is indeed open to scientific debates, by the denial of its need is scientific corruption for personal gain inmaintaining pre-established doctrines.