1 / ((((2 * c) * 376.730313462) / G) / ((4 * pi) / (10^7))) = 3.71295774e-28 kg/m^3
GravitoMagnetic Aether
(3.71295774e-28 kg) * (2 * c) * ((376.730313462 / (4pi/10^7)) / G) = 1
https://en.wikipedia.org/wiki/Unified_field_theory
https://en.wikipedia.org/wiki/Friedmann_equations#Density_parameter
Mass per cubic meter
Black hole = http://vixra.org/pdf/1310.0191vD.pdf
https://sites.google.com/site/lordkronosprime/friedmann-density-kg
((2^0.5) * 376.730313462) / ((0.5 * 3.712958e-28) * kg) = 2.86982572e+30 kg
(2.86982572e+30 kg) / (1 solar mass) = 1.44277599
http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/whdwar.html#c1
Electron Degeneracy
Electron degeneracy is a stellar application of the Pauli Exclusion Principle, as is neutron degeneracy. No two electrons can occupy identical states, even under the pressure of a collapsing star of several solar masses. For stellar masses less than about 1.44 solar masses, the energy from the gravitational collapse is not sufficient to produce the neutrons of a neutron star, so the collapse is halted by electron degeneracy to form white dwarfs. This maximum mass for a white dwarf is called the Chandrasekhar limit. As the star contracts, all the lowest electron energy levels are filled and the electrons are forced into higher and higher energy levels, filling the lowest unoccupied energy levels. This creates an effective pressure which prevents further gravitational collapse.
2.3e+29 Pa
Pressure inside the core of a white dwarf at the Chandrasekhar limit
1 / ((((2^0.5) * pi) * 3.712958e-28 kg) / 376.730313462) = 2.28373475e+29 kg
https://en.wikipedia.org/wiki/Orders_of_magnitude_(pressure)
(29.9792458 * (8^0.5)) / (3.712958e-28 pascals) = 2.28373475e+29 pascals
(1 pascal) / (1 kilogram) = 1 m/s^2
(((2^(7 / 2)) * 376.730313462) / ((2 * G) / (c^2))) / (1 solar mass) = 1.44277609 Solar mass
((2^(7 / 2)) * 376.730313462) / ((2 * G) / (c^2)) =
2.86982592e+30 kg = 1.44 solar mass
(2^(7/2) * (4pi/10^7 henries) / ((2 * G) / (c^3))
http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/whdwar.html
(((8.85418782e-12 * (4pi/10^7)) / 2) * G) * (c^2) = 3.33704e-11 Joules
3.33704e-11 (joules / (meter^3)) = 3.33704e-11 pascals
https://goo.gl/photos/asMLdBuJUK718FPw9
No hair theorem