Page 291 - The Final Appeal to Mankind
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«The Final Appeal to Mankind» by Nicolai Levashov

            3,00017 <  λb < 3,02037323,

            where Δλ may, initially, fluctuate within a range of


            0 < Δλ < 0,020203236...

            Gradually the secondary deformation of the macrospace dimension (due to the star's
            density)  becomes  even  further  pronounced,  causing  the  macrospace  dimension  to
            approximate the value of λ7. As this proceeds, the channel between the λ8 and λ7 space-
            universe diminishes. The flow of matter from λ7 becomes progressively less.

            Concomitantly the star's radiation activity keeps waning until it ceases altogether. This
            marks the death of the star. It grows dimmer and dimmer and finally fades away...

            (see F Fi ig g. .   1 15 58 8, 1 15 59 9).

            By contrast, a star may start out with a huge mass (sixfold that of the sun); then, as it
            wanes, it may trigger a secondary deformation of it macrospace dimension, causing it
            to dip below the value of λ7:

            Δλ ≈ 0.0102018...

            Λ6 < λd < λ7;  λd = λa - Δλ


            The result is an opposite deflection, and a so-called neutron star is born (see F Fi ig g. .   1 15 58 8).

            If, initially, the star had a mass greater than tenfold the mass of the sun, the secondary
            deformation becomes so great as to establish the linkage between space-universes λ7
            and λ6 (see F Fi ig g. .   1 15 59 9).

            When this occurs, matter from λ7 starts flowing over to λ6, resulting in the formation
            of a black hole. Thus, black holes emerge in the course of the evolution of stars.


            Now let us consider how planetary systems are formed.

            At  the  onset  of  its  life  span,  a  star  shows  a  balance  between  its  size,  the  channel
            connecting  λ8 and λ7, and the amount of substance flowing through it from space-
            universe λ8 (see F Fi ig g. .   1 16 60 0).



























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