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  2. Electron degeneracy pressure - Wikipedia

    en.wikipedia.org/wiki/Electron_degeneracy_pressure

    This force is balanced by the electron degeneracy pressure keeping the star stable. [4] In metals, the positive nuclei are partly ionized and spaced by normal interatomic distances. Gravity has negligible effect; the positive ion cores are attracted to the negatively charged electron gas. This force is balanced by the electron degeneracy pressure.

  3. Degenerate matter - Wikipedia

    en.wikipedia.org/wiki/Degenerate_matter

    Above the Chandrasekhar limit, the gravitational pressure at the core exceeds the electron degeneracy pressure, and electrons begin to combine with protons to produce neutrons (via inverse beta decay, also termed electron capture). The result is an extremely compact star composed of "nuclear matter", which is predominantly a degenerate neutron ...

  4. Chandrasekhar limit - Wikipedia

    en.wikipedia.org/wiki/Chandrasekhar_limit

    The Chandrasekhar limit is a consequence of competition between gravity and electron degeneracy pressure. Electron degeneracy pressure is a quantum-mechanical effect arising from the Pauli exclusion principle. Since electrons are fermions, no two electrons can be in the same state, so not all electrons can be in the minimum-energy level.

  5. Degenerate energy levels - Wikipedia

    en.wikipedia.org/wiki/Degenerate_energy_levels

    Some examples of two-dimensional electron systems achieved experimentally include MOSFET, two-dimensional superlattices of Helium, Neon, Argon, Xenon etc. and surface of liquid Helium. The presence of degenerate energy levels is studied in the cases of Particle in a box and two-dimensional harmonic oscillator , which act as useful mathematical ...

  6. Zero field splitting - Wikipedia

    en.wikipedia.org/wiki/Zero_field_splitting

    In quantum mechanics terminology, the degeneracy is said to be "lifted" by the presence of the magnetic field. In the presence of more than one unpaired electron, the electrons mutually interact to give rise to two or more energy states. Zero field splitting refers to this lifting of degeneracy even in the absence of a magnetic field.

  7. Plasma parameters - Wikipedia

    en.wikipedia.org/wiki/Plasma_parameters

    electron gyroradius, the radius of the circular motion of an electron in the plane perpendicular to the magnetic field: = ion gyroradius , the radius of the circular motion of an ion in the plane perpendicular to the magnetic field: r i = v T i ω c i ≈ 1.02 × 10 2 ( μ T i ) 1 2 Z B cm {\displaystyle r_{i}={\frac {v_{Ti}}{\omega _{ci ...

  8. Stark effect - Wikipedia

    en.wikipedia.org/wiki/Stark_effect

    The one-electron states with even are even under parity, while those with odd are odd under parity. Hence hydrogen-like atoms with n >1 show first-order Stark effect. The first-order Stark effect occurs in rotational transitions of symmetric top molecules (but not for linear and asymmetric molecules).

  9. Fermi liquid theory - Wikipedia

    en.wikipedia.org/wiki/Fermi_liquid_theory

    The Fermi liquid is qualitatively analogous to the non-interacting Fermi gas, in the following sense: The system's dynamics and thermodynamics at low excitation energies and temperatures may be described by substituting the non-interacting fermions with interacting quasiparticles, each of which carries the same spin, charge and momentum as the original particles.