Loren Booda
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My two cents, from http://www.quantumdream.net :
The "Hubble acceleration," aH=c2/RH=cH0=6 x 10-8 cm/s2, demarcates a critical radial acceleration for galaxies and larger bodies where the influence of so-called dark matter begins. Following the rotation curve for a given galaxy, one notices the departure from conventional luminous matter dynamics at approximately the rotational velocity v with radius r so that aH=v2/r. This asserts that the radial universal expansion parameters, i. e., the Hubble acceleration, also affect rotational dynamics. The concept of "dark matter" may arise in large part to a quantizing of aH. If so, this would indicate a characteristic of baryonic matter's inertia to overcome an "ultraviolet catastrophe" (similar to the blackbody's). Consequently, it tends to maintain the acceleration, and likewise the velocity, of galaxies' outlying halos.
The effects of "dark matter" on large-scale structures are predominantly due to compliance with discretized minimal acceleration, given by the ratio between speed of light squared and the cosmological horizon radius.
The "Hubble acceleration," aH=c2/RH=cH0=6 x 10-8 cm/s2, demarcates a critical radial acceleration for galaxies and larger bodies where the influence of so-called dark matter begins. Following the rotation curve for a given galaxy, one notices the departure from conventional luminous matter dynamics at approximately the rotational velocity v with radius r so that aH=v2/r. This asserts that the radial universal expansion parameters, i. e., the Hubble acceleration, also affect rotational dynamics. The concept of "dark matter" may arise in large part to a quantizing of aH. If so, this would indicate a characteristic of baryonic matter's inertia to overcome an "ultraviolet catastrophe" (similar to the blackbody's). Consequently, it tends to maintain the acceleration, and likewise the velocity, of galaxies' outlying halos.
The effects of "dark matter" on large-scale structures are predominantly due to compliance with discretized minimal acceleration, given by the ratio between speed of light squared and the cosmological horizon radius.
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