Why is there an upper limit to the mass that can be supported by electron degeneracy pressure?

Electron degeneracy pressure is a specific manifestation of the more general occurrence of quantum degeneracy pressure. What is mass electron degeneracy pressure?Electron degeneracy pressure will halt the gravitational slump of a star if its mass is below the Chandrasekhar limit (1.44 solar masses). This is the pressure that averts a white dwarf star from collapsing. Electron degeneracy pressure occurs when electrons are squeezed into a very small volume. Since their positions are well-known, they gain a large momentum in obedience to Heisenberg's uncertainty principle. This momentum generates a pressure that is temperature-independent and can result in helium flash. in stars. Electron degeneracy occurs at a solidity of about 106 kg/m3. So we can conclude that  The electron degeneracy pressure is taken by (n.v.p) where n is the number density, and v is the mean speed of the degenerate electrons.Learn more about Electron degeneracy here: https://brainly.com/question/14439838#SPJ1