As a result, when they are tightly packed, they exhibit a strong quantum-mechanical degeneracy pressure responsible for the stability of white dwarves and neutron stars.
They are characterized by a wave function which is anti-symmetric under the operator representing particle interchange. As a result, when they are tightly packed, they exhibit a strong quantum-mechanical degeneracy pressure responsible for the stability of white dwarves and neutron stars. They include all leptons, baryons, and quarks, because they all have half-integer spin. FTP, name this class of particles which obey the Pauli exclusion principle, consisting of anything which is not a boson.
They are characterized by a wave function which is anti-symmetric under the operator representing particle interchange.
fermions