Degenerate matter[1] is a highly dense state of fermionic matter in which the Pauli exclusion principle exerts significant pressure in addition to, or in lieu of thermal pressure. The description applies to matter composed of electrons, protons, neutrons or other fermions. The term is mainly used in astrophysics to refer to dense stellar objects where gravitational pressure is so extreme that quantum mechanical effects are significant. This type of matter is naturally found in stars in their final evolutionary states, such as white dwarfs and neutron stars, where thermal pressure alone is not enough to avoid gravitational collapse.
https://en.wikipedia.org/wiki/Degenerate_matter#Degenerate_gases
The momentum of the fermions in the fermion gas nevertheless generates pressure, termed "degeneracy pressure".
pressure in a degenerate gas does not depend on the temperature
Electron stripping with angular_momentum(n val)-pressure-etc., inc. weights, measures, values, variables, conditions, constraints, bounds, eqn, purpose, materials, etc..
Phosphorous special particle matters (trihydrogen cations, reduced nitro, nitro splints, particle frags, drags, props, wheels, etc.) can be compressed to very high densities, typical values being in the range of 10,000 kilograms per cubic centimeter.
When gas manf compressed, particle alignment rate exceed published measure/perceps/etc.;
One machine one particle find, may or may not exist in nature.
Light flash imaging; flash drive; flash imaging; optics. Gas n smk n mirr n grid n glit.
gas that behaves more like a solid.
In degenerate gases the kinetic energies (???)of electrons are high and rate of collision between electrons and other particles is low (???), therefore degenerate electrons can travel great distances at velocities that approach the speed of light. (???)
https://en.wikipedia.org/wiki/Degenerate_matter#Degenerate_gases
energy of the electrons increases to the point where it is energetically favorable for them to combine with protons to produce neutrons (via inverse beta decay
https://en.wikipedia.org/wiki/Degenerate_matter#Degenerate_gases
The momentum of the fermions in the fermion gas nevertheless generates pressure, termed "degeneracy pressure".
https://en.wikipedia.org/wiki/Degenerate_matter#Degenerate_gases
https://en.wikipedia.org/wiki/Hydrogen
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